diff --git a/CLAUDE.md b/CLAUDE.md index a543f1b..f80cf68 100644 --- a/CLAUDE.md +++ b/CLAUDE.md @@ -72,8 +72,7 @@ Tbx ├── Sc # ├── Ph # ├── Title # -├── Namespaces # XML namespace definitions -└── Ruby # Gem namespace (Tbx::Ruby::VERSION) +└── Namespace # XML namespace definition (urn:iso:std:iso:30042:ed-2) ``` ### Key Implementation Patterns @@ -95,7 +94,7 @@ module Tbx xml do root "conceptEntry" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "langSec", to: :lang_sec @@ -108,7 +107,7 @@ end ### XML Namespace -The TBX namespace is `urn:iso:std:iso:30042:ed-2` defined in `Tbx::Namespaces::TbxNamespace`. +The TBX namespace is `urn:iso:std:iso:30042:ed-2` defined in `Tbx::Namespace`. ### TBX Styles diff --git a/Gemfile b/Gemfile index 37b15ac..efaf4b6 100644 --- a/Gemfile +++ b/Gemfile @@ -5,7 +5,7 @@ source "https://rubygems.org" gemspec gem "canon" -gem "lutaml-model", path: "../../lutaml/lutaml-model" +gem "lutaml-model", github: "lutaml/lutaml-model", branch: "main" gem "nokogiri" gem "rake", "~> 13.0" gem "rspec", "~> 3.0" diff --git a/lib/tbx.rb b/lib/tbx.rb index de2c46f..934c550 100644 --- a/lib/tbx.rb +++ b/lib/tbx.rb @@ -4,7 +4,7 @@ require_relative "tbx/version" module Tbx - autoload :Namespaces, "#{__dir__}/tbx/namespaces" + autoload :Namespace, "#{__dir__}/tbx/namespace" # Inline elements autoload :Ec, "#{__dir__}/tbx/ec" diff --git a/lib/tbx/admin.rb b/lib/tbx/admin.rb index 14bbdbe..4acc9e7 100644 --- a/lib/tbx/admin.rb +++ b/lib/tbx/admin.rb @@ -17,7 +17,7 @@ class Admin < Lutaml::Model::Serializable xml do root "admin" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/admin_grp.rb b/lib/tbx/admin_grp.rb index dbd8c71..c835ba6 100644 --- a/lib/tbx/admin_grp.rb +++ b/lib/tbx/admin_grp.rb @@ -12,7 +12,7 @@ class AdminGrp < Lutaml::Model::Serializable xml do root "adminGrp" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "admin", to: :admin diff --git a/lib/tbx/admin_note.rb b/lib/tbx/admin_note.rb index 5a0b012..32523a2 100644 --- a/lib/tbx/admin_note.rb +++ b/lib/tbx/admin_note.rb @@ -12,7 +12,7 @@ class AdminNote < Lutaml::Model::Serializable xml do root "adminNote" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/back.rb b/lib/tbx/back.rb index c86dabc..b64967a 100644 --- a/lib/tbx/back.rb +++ b/lib/tbx/back.rb @@ -8,7 +8,7 @@ class Back < Lutaml::Model::Serializable xml do root "back" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "refObjectSec", to: :ref_object_sec diff --git a/lib/tbx/body.rb b/lib/tbx/body.rb index 5520c38..785ee7d 100644 --- a/lib/tbx/body.rb +++ b/lib/tbx/body.rb @@ -8,7 +8,7 @@ class Body < Lutaml::Model::Serializable xml do root "body" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "conceptEntry", to: :concept_entry diff --git a/lib/tbx/change.rb b/lib/tbx/change.rb index f751b53..6fe7c3c 100644 --- a/lib/tbx/change.rb +++ b/lib/tbx/change.rb @@ -9,7 +9,7 @@ class Change < Lutaml::Model::Serializable xml do root "change" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/concept_entry.rb b/lib/tbx/concept_entry.rb index 7bf18a4..4354866 100644 --- a/lib/tbx/concept_entry.rb +++ b/lib/tbx/concept_entry.rb @@ -16,7 +16,7 @@ class ConceptEntry < Lutaml::Model::Serializable xml do root "conceptEntry" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "admin", to: :admin diff --git a/lib/tbx/date.rb b/lib/tbx/date.rb index 05895e3..741f832 100644 --- a/lib/tbx/date.rb +++ b/lib/tbx/date.rb @@ -7,7 +7,7 @@ class DateElement < Lutaml::Model::Serializable xml do root "date" - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_content to: :content diff --git a/lib/tbx/descrip.rb b/lib/tbx/descrip.rb index dd730e0..45b2e8e 100644 --- a/lib/tbx/descrip.rb +++ b/lib/tbx/descrip.rb @@ -17,7 +17,7 @@ class Descrip < Lutaml::Model::Serializable xml do root "descrip" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/descrip_grp.rb b/lib/tbx/descrip_grp.rb index eb72520..9567c47 100644 --- a/lib/tbx/descrip_grp.rb +++ b/lib/tbx/descrip_grp.rb @@ -15,7 +15,7 @@ class DescripGrp < Lutaml::Model::Serializable xml do root "descripGrp" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "descrip", to: :descrip diff --git a/lib/tbx/descrip_note.rb b/lib/tbx/descrip_note.rb index a953078..facb1a3 100644 --- a/lib/tbx/descrip_note.rb +++ b/lib/tbx/descrip_note.rb @@ -12,7 +12,7 @@ class DescripNote < Lutaml::Model::Serializable xml do root "descripNote" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/document.rb b/lib/tbx/document.rb index 836c541..0dc61c5 100644 --- a/lib/tbx/document.rb +++ b/lib/tbx/document.rb @@ -11,7 +11,7 @@ class Document < Lutaml::Model::Serializable xml do root "tbx" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace w3c_attributes :lang map_attribute "type", to: :type diff --git a/lib/tbx/ec.rb b/lib/tbx/ec.rb index 42ce34c..c67ee4d 100644 --- a/lib/tbx/ec.rb +++ b/lib/tbx/ec.rb @@ -13,7 +13,7 @@ class Ec < Lutaml::Model::Serializable xml do root "ec" - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "startRef", to: :start_ref map_attribute "isolated", to: :isolated diff --git a/lib/tbx/encoding_desc.rb b/lib/tbx/encoding_desc.rb index c0fe5e0..a505e80 100644 --- a/lib/tbx/encoding_desc.rb +++ b/lib/tbx/encoding_desc.rb @@ -8,7 +8,7 @@ class EncodingDesc < Lutaml::Model::Serializable xml do root "encodingDesc" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "p", to: :p diff --git a/lib/tbx/file_desc.rb b/lib/tbx/file_desc.rb index c0cccd7..73fd7bb 100644 --- a/lib/tbx/file_desc.rb +++ b/lib/tbx/file_desc.rb @@ -10,7 +10,7 @@ class FileDesc < Lutaml::Model::Serializable xml do root "fileDesc" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "publicationStmt", to: :publication_stmt diff --git a/lib/tbx/foreign.rb b/lib/tbx/foreign.rb index 3898e2b..cf2afc4 100644 --- a/lib/tbx/foreign.rb +++ b/lib/tbx/foreign.rb @@ -14,7 +14,7 @@ class Foreign < Lutaml::Model::Serializable xml do root "foreign" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/hi.rb b/lib/tbx/hi.rb index 2f8e582..2510ad7 100644 --- a/lib/tbx/hi.rb +++ b/lib/tbx/hi.rb @@ -9,7 +9,7 @@ class Hi < Lutaml::Model::Serializable xml do root "hi" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "target", to: :target map_attribute "type", to: :type diff --git a/lib/tbx/item.rb b/lib/tbx/item.rb index 852596e..6cd0cad 100644 --- a/lib/tbx/item.rb +++ b/lib/tbx/item.rb @@ -14,7 +14,7 @@ class Item < Lutaml::Model::Serializable xml do root "item" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_attribute "type", to: :type diff --git a/lib/tbx/item_grp.rb b/lib/tbx/item_grp.rb index cebe8ac..7cc2c02 100644 --- a/lib/tbx/item_grp.rb +++ b/lib/tbx/item_grp.rb @@ -14,7 +14,7 @@ class ItemGrp < Lutaml::Model::Serializable xml do root "itemGrp" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "item", to: :item diff --git a/lib/tbx/item_set.rb b/lib/tbx/item_set.rb index 06a1f70..4e5de97 100644 --- a/lib/tbx/item_set.rb +++ b/lib/tbx/item_set.rb @@ -10,7 +10,7 @@ class ItemSet < Lutaml::Model::Serializable xml do root "itemSet" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_attribute "type", to: :type diff --git a/lib/tbx/lang_sec.rb b/lib/tbx/lang_sec.rb index c6ab9c1..633773e 100644 --- a/lib/tbx/lang_sec.rb +++ b/lib/tbx/lang_sec.rb @@ -16,7 +16,7 @@ class LangSec < Lutaml::Model::Serializable xml do root "langSec" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace w3c_attributes :lang map_element "admin", to: :admin diff --git a/lib/tbx/namespace.rb b/lib/tbx/namespace.rb new file mode 100644 index 0000000..afb355e --- /dev/null +++ b/lib/tbx/namespace.rb @@ -0,0 +1,7 @@ +# frozen_string_literal: true + +module Tbx + class Namespace < Lutaml::Xml::Namespace + uri "urn:iso:std:iso:30042:ed-2" + end +end diff --git a/lib/tbx/namespaces.rb b/lib/tbx/namespaces.rb deleted file mode 100644 index ab1a2fb..0000000 --- a/lib/tbx/namespaces.rb +++ /dev/null @@ -1,9 +0,0 @@ -# frozen_string_literal: true - -module Tbx - module Namespaces - class TbxNamespace < Lutaml::Xml::Namespace - uri "urn:iso:std:iso:30042:ed-2" - end - end -end diff --git a/lib/tbx/note.rb b/lib/tbx/note.rb index ceb349d..4401e2d 100644 --- a/lib/tbx/note.rb +++ b/lib/tbx/note.rb @@ -14,7 +14,7 @@ class Note < Lutaml::Model::Serializable xml do root "note" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/p.rb b/lib/tbx/p.rb index 1e9b8d8..378dab6 100644 --- a/lib/tbx/p.rb +++ b/lib/tbx/p.rb @@ -15,7 +15,7 @@ class P < Lutaml::Model::Serializable xml do root "p" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/ph.rb b/lib/tbx/ph.rb index b9867c9..75ac750 100644 --- a/lib/tbx/ph.rb +++ b/lib/tbx/ph.rb @@ -6,7 +6,7 @@ class Ph < Lutaml::Model::Serializable xml do root "ph" - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "type", to: :type end diff --git a/lib/tbx/publication_stmt.rb b/lib/tbx/publication_stmt.rb index 91cf4b6..2aac4d0 100644 --- a/lib/tbx/publication_stmt.rb +++ b/lib/tbx/publication_stmt.rb @@ -8,7 +8,7 @@ class PublicationStmt < Lutaml::Model::Serializable xml do root "publicationStmt" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "p", to: :p diff --git a/lib/tbx/ref.rb b/lib/tbx/ref.rb index 21ab74b..d1e0f81 100644 --- a/lib/tbx/ref.rb +++ b/lib/tbx/ref.rb @@ -12,7 +12,7 @@ class Ref < Lutaml::Model::Serializable xml do root "ref" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/ref_object.rb b/lib/tbx/ref_object.rb index 7e0dc50..5d7c15e 100644 --- a/lib/tbx/ref_object.rb +++ b/lib/tbx/ref_object.rb @@ -10,7 +10,7 @@ class RefObject < Lutaml::Model::Serializable xml do root "refObject" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "itemSet", to: :item_set diff --git a/lib/tbx/ref_object_sec.rb b/lib/tbx/ref_object_sec.rb index e3a44f1..cedc550 100644 --- a/lib/tbx/ref_object_sec.rb +++ b/lib/tbx/ref_object_sec.rb @@ -9,7 +9,7 @@ class RefObjectSec < Lutaml::Model::Serializable xml do root "refObjectSec" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_attribute "type", to: :type diff --git a/lib/tbx/revision_desc.rb b/lib/tbx/revision_desc.rb index 06c0608..bbd041a 100644 --- a/lib/tbx/revision_desc.rb +++ b/lib/tbx/revision_desc.rb @@ -9,7 +9,7 @@ class RevisionDesc < Lutaml::Model::Serializable xml do root "revisionDesc" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/sc.rb b/lib/tbx/sc.rb index 782d4f7..7ea1748 100644 --- a/lib/tbx/sc.rb +++ b/lib/tbx/sc.rb @@ -10,7 +10,7 @@ class Sc < Lutaml::Model::Serializable xml do root "sc" - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_attribute "isolated", to: :isolated diff --git a/lib/tbx/source_desc.rb b/lib/tbx/source_desc.rb index 81e9621..8ce6618 100644 --- a/lib/tbx/source_desc.rb +++ b/lib/tbx/source_desc.rb @@ -9,7 +9,7 @@ class SourceDesc < Lutaml::Model::Serializable xml do root "sourceDesc" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/tbx_header.rb b/lib/tbx/tbx_header.rb index 57fcc4d..c9178b1 100644 --- a/lib/tbx/tbx_header.rb +++ b/lib/tbx/tbx_header.rb @@ -10,7 +10,7 @@ class TbxHeader < Lutaml::Model::Serializable xml do root "tbxHeader" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "fileDesc", to: :file_desc diff --git a/lib/tbx/term.rb b/lib/tbx/term.rb index 381d14d..ec0b8ce 100644 --- a/lib/tbx/term.rb +++ b/lib/tbx/term.rb @@ -9,7 +9,7 @@ class Term < Lutaml::Model::Serializable xml do root "term" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_content to: :content diff --git a/lib/tbx/term_note.rb b/lib/tbx/term_note.rb index 1dea926..8d27091 100644 --- a/lib/tbx/term_note.rb +++ b/lib/tbx/term_note.rb @@ -17,7 +17,7 @@ class TermNote < Lutaml::Model::Serializable xml do root "termNote" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/term_note_grp.rb b/lib/tbx/term_note_grp.rb index e0864e5..91cffb3 100644 --- a/lib/tbx/term_note_grp.rb +++ b/lib/tbx/term_note_grp.rb @@ -14,7 +14,7 @@ class TermNoteGrp < Lutaml::Model::Serializable xml do root "termNoteGrp" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "termNote", to: :term_note diff --git a/lib/tbx/term_sec.rb b/lib/tbx/term_sec.rb index 841fcb5..8d98ea0 100644 --- a/lib/tbx/term_sec.rb +++ b/lib/tbx/term_sec.rb @@ -18,7 +18,7 @@ class TermSec < Lutaml::Model::Serializable xml do root "termSec" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "term", to: :term diff --git a/lib/tbx/text_element.rb b/lib/tbx/text_element.rb index 8d04c33..6a67f5a 100644 --- a/lib/tbx/text_element.rb +++ b/lib/tbx/text_element.rb @@ -9,7 +9,7 @@ class TextElement < Lutaml::Model::Serializable xml do root "text" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "body", to: :body diff --git a/lib/tbx/title.rb b/lib/tbx/title.rb index efc5653..d4a1ec6 100644 --- a/lib/tbx/title.rb +++ b/lib/tbx/title.rb @@ -9,7 +9,7 @@ class Title < Lutaml::Model::Serializable xml do root "title" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/title_stmt.rb b/lib/tbx/title_stmt.rb index 97dd6c7..d1d0665 100644 --- a/lib/tbx/title_stmt.rb +++ b/lib/tbx/title_stmt.rb @@ -10,7 +10,7 @@ class TitleStmt < Lutaml::Model::Serializable xml do root "titleStmt" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/transac.rb b/lib/tbx/transac.rb index f34d88f..974fe0c 100644 --- a/lib/tbx/transac.rb +++ b/lib/tbx/transac.rb @@ -12,7 +12,7 @@ class Transac < Lutaml::Model::Serializable xml do root "transac" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/transac_grp.rb b/lib/tbx/transac_grp.rb index 67e2c8b..9abdcbd 100644 --- a/lib/tbx/transac_grp.rb +++ b/lib/tbx/transac_grp.rb @@ -13,7 +13,7 @@ class TransacGrp < Lutaml::Model::Serializable xml do root "transacGrp" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_element "transac", to: :transac diff --git a/lib/tbx/transac_note.rb b/lib/tbx/transac_note.rb index 4d5aab5..9beefe6 100644 --- a/lib/tbx/transac_note.rb +++ b/lib/tbx/transac_note.rb @@ -12,7 +12,7 @@ class TransacNote < Lutaml::Model::Serializable xml do root "transacNote" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id w3c_attributes :lang diff --git a/lib/tbx/xref.rb b/lib/tbx/xref.rb index e1c3184..6c8c68c 100644 --- a/lib/tbx/xref.rb +++ b/lib/tbx/xref.rb @@ -10,7 +10,7 @@ class Xref < Lutaml::Model::Serializable xml do root "xref" mixed_content - namespace ::Tbx::Namespaces::TbxNamespace + namespace ::Tbx::Namespace map_attribute "id", to: :id map_attribute "target", to: :target diff --git a/spec/fixtures/TBX_test_files b/spec/fixtures/TBX_test_files deleted file mode 160000 index ba0e7bc..0000000 --- a/spec/fixtures/TBX_test_files +++ /dev/null @@ -1 +0,0 @@ -Subproject commit ba0e7bc69f596c48e2d5963c68029b09e07dceef diff --git a/spec/fixtures/TBX_test_files/README.adoc b/spec/fixtures/TBX_test_files/README.adoc new file mode 100644 index 0000000..8c1cc6f --- /dev/null +++ b/spec/fixtures/TBX_test_files/README.adoc @@ -0,0 +1,24 @@ += TBX Test Files + +These test files are sourced from the +https://github.com/LTAC-Global/TBX_test_files[TBX_test_files] repository +maintained by https://ltac-global.org[LTAC Global]. + +== Purpose + +These files demonstrate TBX validation across different dialect levels: + +* `core_structure_good.tbx` / `core_structure_bad.tbx` -- TBX core structure validation +* `min_good.tbx` / `min_bad.tbx` -- TBX-Min dialect validation +* `basic_good.tbx` / `basic_bad.tbx` -- TBX-Basic dialect validation +* `poorly_formed_xml.tbx` -- general XML well-formedness check + +== License + +These test files are made available by LTAC Global for testing and validation +purposes. See the upstream repository for license details. + +== Acknowledgments + +Thank you to LTAC Global for making these test files publicly available for +the TBX community. diff --git a/spec/fixtures/TBX_test_files/README.md b/spec/fixtures/TBX_test_files/README.md new file mode 100644 index 0000000..dc04d13 --- /dev/null +++ b/spec/fixtures/TBX_test_files/README.md @@ -0,0 +1,46 @@ +# These are test files +These files are intended to show how to validate TBX files from different dialects. At each level, there is a file that is valid and a file that should be rejected by that dialect's schema. The demonstrated dialects are TBX-Min and TBX-Basic, which are detailed [on the TBX website](https://www.tbxinfo.net/tbx-modules/). There are also files specifically for validation against the TBX core structure, as well as one for general XML well-formedness. + +To validate any TBX file, you will need to have either core_schema.rng or core_schema.xsd downloaded. This ReadMe uses core_schema.rng, but either should work fine. Both of these files, as well as min_schema.sch and basic_schema.sch, will soon be posted in a location that will be referenced here. + +# How to validate with oXygen +First, **open the TBX file** to validate in oXygen. + +Then, **associate the TBX file** with applicable schemas against which it will be validated. For all dialects you will need to validate against the **TBX core structure**. Insert the following line of XML at the top of your TBX file, above the opening tag of the `<tbx>` element; replace `PATH` with the relative filepath from the TBX file to wherever you have placed the `core_schema.rng` file: + +`<?xml-model href="PATH/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?>` + +For TBX-Min, TBX-Basic, or any other dialect, there are **Schematron rules** to associate in addition to the TBX core structure. Add the following XML just after the line for the core structure, again replacing `PATH` with the relative filepath from the TBX file to the Schematron file (for TBX-Min and TBX-Basic, this would be min_schema.sch and basic_schema.sch, respectively): + +`<?xml-model href="PATH" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?>` + +Finally, **validate the TBX file** by clicking the icon on the top toolbar which shows a page with a big red checkmark on it. Any errors will be displayed at the bottom of the screen. Success will yield a green square and a success message. + +# How to validate without oXygen +If you don't have the full paid version of oXygen, you can use a free tool like Liquid Studio. This can be found [online](https://www.liquid-technologies.com/online-relaxng-validator) or the community edition can be [downloaded for free](https://www.liquid-technologies.com/trial-download). + +## Using Liquid Studio online +### Validating against the TBX-Core +On the webpage linked above: +1. select either `XML Validator (RelaxNG)` or `XML Validator (XSD)` on the left side, depending on whether you are using core_schema.rng or core_schema.xsd. +2. Copy and paste the whole contents of your TBX file into the box labelled `XML data to validate`. +3. Copy and paste the whole RNG or XSD file containing the TBX core structure in the box labelled `RelaxNG data` or `XML schema (XSD) data`. +4. Fill out the captcha and press `validate`. + +### Validating against a dialect +To validate against a dialect, such as TBX-Min or TBX-Basic, first follow the steps above to validate against the TBX core structure. Then: +1. Select `XML Validator (Schematron)` on the left side of the webpage. +2. Copy and paste the whole contents of your TBX file into the box labelled `XML data to validate`. +3. Copy and paste the whole Schematron file containing your dialect's rules in the box labelled `Schematron data`. +4. Fill out the captcha and press `validate`. + +## Using Liquid Studio Community Edition +To download and use a free tool from your desktop: +1. Follow the instructions [here](https://www.liquid-technologies.com/trial-download). +2. Open your TBX file in Liquid Studio +3. Associate the file with the core structure schema by inserting the following line of XML at the top of your TBX file, above the opening tag of the `<tbx>` element; replace `PATH` with the relative filepath from the TBX file to wherever you have placed the `core_schema.rng` file: + +`<?xml-model href="PATH/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?>` + +4. If the file uses a dialect, associate it with that dialect's Schematron: click `Schema Used to Validate XML1` or use `Ctrl + F7` to open the Schema Mapping Menu. Under `XML Schema Files`, click `Additional Schemas` and then `Add Schema File`. Find and select your dialect's Schematron file, then close the window with `OK` +5. Click `Validate Document` or use `F7` to validate. A dialog box will show results. diff --git a/spec/fixtures/TBX_test_files/basic_bad.tbx b/spec/fixtures/TBX_test_files/basic_bad.tbx new file mode 100644 index 0000000..e6a2df6 --- /dev/null +++ b/spec/fixtures/TBX_test_files/basic_bad.tbx @@ -0,0 +1,4038 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<?xml-model href="../../schematrons/basic_schema.sch" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?> +<!-- + Expected errors: + - "source" at concept level, not nested in a descripGrp (would have to be grouped with a "definition") + - "definition" decleared at term level + - "partOfSpeech" value not adhering to picklist + - <transacNote> of @type other than "responsibility" + - <transac> of @type other than "transactionType" +--> +<tbx type="TBX-Basic" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + + <text> + <body> + <conceptEntry id="c1"> + <admin type="source">Wrong level to have no nesting at.</admin> + <transacGrp> + <transac type="theWrongType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Galaxy_cluster#/media/File:Galaxy_cluster_IDCS_J1426.jpg">Open_Cluster.JPG</xref> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A group of stars formed together in the spiral + arms of a galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>open cluster</term> + + + <termNote type="partOfSpeech">nominal</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Over 1100 open clusters are known in our Milky + Way Galaxy, and this is probably only a small percentage of the + total population which is probably some factor higher; estimates of + as many as about 100,000 Milky Way open clusters have been given. </descrip> + <admin type="source">http://seds.org/MESSIER/open.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>galactic cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <descripGrp> + <descrip type="context">In contrast, the galactic cluster represented by + M29 is a grouping of stars—a “knot” of stars in the stellar + backdrop.</descrip> + <admin type="source">http://www.eastbayastro.org/2000/0900/r0900-8.htm</admin> + </descripGrp> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + <descrip type="definition">Definitions may not go at the term level.</descrip> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una acumulación de una docena hasta varios miles + de jóvenes estrellas en el plano de las galaxias.</descrip> + <admin type="source">http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Cumulo_abierto.html</admin> + </descripGrp> + <termSec> + <term>cúmulo abierto</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">M7 es uno de los cúmulos abiertos estelares más + prominentes del cielo. El cúmulo, dominado por brillantes estrellas + azules, puede ser visto a ojo desnudo en un cielo oscuro en la cola + de la constelación del Escorpión (Scorpius).Contiene unas 100 + estrellas en total, tiene una edad aproximada de 200 millones de + años, mide 25 años luz de ancho, y se encuentra a unos 1000 años luz + de distancia.</descrip> + <admin type="source">http://observatorio.info/2009/11/m7-cumulo-abierto-en-scorpius-2/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c2"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="wrongType" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Accretion_disk#/media/File:Star_with_accretion_disk.jpg">Accretion_Disk.jpg</xref> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A structure that forms around a compact object + (e.g. a white dwarf, neutron star, or black hole) when matter flows + towards it.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>circumstellar accretion disk</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">In contrast with the violence of merging, the + gradual growth of massive stars by accretion is likely to produce + less infrared variability, relatively thin circumstellar accretion + disks that maintain their orientation, and collimated bipolar + outflows that are scaled-up versions of those produced by low-mass + young stellar objects.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>accretion disc</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Accretion Disc Evolution in Single and Binary T + Tauri Stars</descrip> + <admin type="source">http://cdsweb.cern.ch/record/369655</admin> + </descripGrp> + </termSec> + <termSec> + <term>circumstellar disk</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Our results suggest a scenario of a central star + accreting material from a circumstellar disc at the centre of a cool + extended rotating torus, while driving a fast bipolar wind. </descrip> + <admin type="source">http://adsabs.harvard.edu/abs/2010MNRAS.402.1504D</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estructura en forma de disco alrededor de un + objeto central masivo que alimenta el cuerpo central siendo atraido por + éste y contribuye a su aumento de masa.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Disco_de_acreci%C3%B3n</admin> + </descripGrp> + <termSec> + <term>disco de acreción</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Lo que alimenta esta actividad es el gas + extraído de la estrella normal, que, cayendo en espiral hacia el + agujero negro, se acumula en un denso disco de acreción.</descrip> + <admin type="source">http://www.amazings.com/ciencia/noticias/010210e.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Imágenes de estrellas jóvenes con discos de + acrecimeinto y chorros colimados de material, tomadas con el + telescopio espacial Hubble.</descrip> + <admin type="source">http://www.laeff.inta.es/index.php?op=modload&name=phpWiki&file=index&pagename=Research-Brown%20Dwarfs-BD_esp-DiscosAcrecimiento</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c3"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Black_hole#/media/File:BH_LMC.png">Black_Hole.jpg</xref> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A region of space where the gravitational force + is so strong that not even light can escape from it.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>black hole</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">As matter spirals toward and into the black + hole, some of its gravitational potential energy may be efficiently + converted into relativistic jets launched by the magnetic field + along the spin axis.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un punto super-denso en el espacio formado por el + colapso de una estrella donde nada puede escapar de su influencia + gravitacional. </descrip> + <admin type="source">www.atlasoftheuniverse.com/espanol/glossary.html</admin> + </descripGrp> + <termSec> + <term>agujero negro</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En teoría un agujero negro se origina hacia el + final de la vida de una estrella, cuando ésta se contrae mas allá de + un límite determinado - conocido como radio de Schwarzschild - y se + hace más pequeña y mas densa que una estrella de neutrones, tanto + que ni la luz puede escapar de su campo gravitatorio.</descrip> + <admin type="source">http://html.rincondelvago.com/agujeros-negros_5.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c4"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Gamma-ray_burst#/media/File:GRB080319B_illustration_NASA.jpg">Gamma_Ray_Burst.jpg</xref> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A temporary intese burst of gamma rays and X-rays + from a cosmic source.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>gamma-ray burst</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>GRB</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">acronym</termNote> + <descripGrp> + <descrip type="context">The off-axis collisions and merging of stars + near the top of the stellar mass spectrum may result in the + production of GRBs.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Destellos de rayos gamma que pueden durar desde + unos nanosegundos hasta cerca de una hora.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Brote_de_rayos_gamma</admin> + </descripGrp> + <termSec> + <term>explosión de rayos gamma</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Una poderosa explosión de rayos gamma, detectada + el 19 de marzo por el satélite Swift, de la NASA, batió el récord + como el objeto más distante que se pudo observar a simple + vista.</descrip> + <admin type="source">http://ciencia.nasa.gov/headlines/y2008/21mar_nakedeye.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">John Ellis (entrevistado por Punset en su + despacho en el CERN en un programa de Redes) y sus colaboradores + mostraron cómo utilizar las propiedades de los grandes brotes de + rayos gamma (gamma-ray bursters o GRBs) para responder a esta + cuestión.</descrip> + <admin type="source">http://francisthemulenews.wordpress.com/2009/02/21/el-mayor-brote-de-rayos-gamma-grb-080916c-acerca-la-gravedad-cuantica-al-mundo-de-planck/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c5"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Globular_cluster#/media/File:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg">Globular_Cluster.jpg</xref> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A roughly spherical group of old stars in the + halo of the galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>globular cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Although the standard accretion scenario may + well explain the formation of most massive stars, the existence of + blue stragglers in globular clusters indicates that mergers do occur + in nature.</descrip> + <admin type="source">Birth of High-Mass Stars</admin> + </descripGrp> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un tipo de cúmulo estelar que consiste en una + agrupación de miles de estrellas viejas, gravitacionalmente ligadas, con + distribución aproximadamente esférica, y que orbita en torno a una + galaxia de manera similar a un satélite.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/C%C3%BAmulo_globular</admin> + </descripGrp> + <termSec> + <term>cúmulo globular</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context"> De los 200 cúmulos globulares que sobreviven + hoy, M3 es uno de los más grande y luminoso, fácilmente observable + con binoculares en el hemisferio Norte del cielo.</descrip> + <admin type="source">http://www.tayabeixo.org/portadas/m3.htm</admin> + </descripGrp> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c6"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Main_sequence#/media/File:HRDiagram.png">Main_Sequence.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <descripGrp> + <descrip type="definition">Of or dealing with a major group of stars forming + a band stretching from upper left to lower right on a + Hertzsprung-Russell diagram when being plotted by luminosity and surface + temperature.</descrip> + <admin type="source">http://en.wiktionary.org/wiki/main-sequence</admin> + </descripGrp> + <termSec> + <term>main-sequence</term> + + + <termNote type="partOfSpeech">adjective</termNote> + <descripGrp> + <descrip type="context">However, immediately after its formation, the + merger product is likely to have a photospheric radius considerably + larger than that of a main-sequence star with the same + mass.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Pertenece a las estrellas en la región del + diagrama de Hertzsprung-Russell en la que se encuentran la mayor parte + de las estrellas que transforman hidrógeno en helio.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Secuencia_principal</admin> + </descripGrp> + <termSec> + <term>de secuencia principal</term> + + + <termNote type="partOfSpeech">adjective</termNote> + <descripGrp> + <descrip type="context">Por ejemplo, nuestro sol es una estrella de + secuencia principal regular de tamaño pequeño. </descrip> + <admin type="source">http://celestia.albacete.org/celestia/celestia/stars/secu5.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c7"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Protostar#/media/File:A_diamond_in_the_dust.jpg">Protostar.JPG</xref> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A star in the earliest observable stage of + formation.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>protostar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Alternatively, it has been suggested that + massive stars form from the merging of lower mass protostars in + high-density protostar clusters (Bonnell et al.1998; Stahler et al. + 2000; Bonnell 2002; Zinnecker & Bate 2002).</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <descripGrp> + <descrip type="definition">Una región muy densa o descorazonada de nubes + moleculares donde existen estrellas en proceso de formación.</descrip> + <admin type="source">www.astrocosmo.cl/glosario/glosar-p.htm</admin> + </descripGrp> + <termSec> + <term>protoestrella</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En estos primeros estadios, la protoestrella es + un objeto muy activo, y produce un viento bipolar formado por dos + chorros opuestos de material de alta velocidad. </descrip> + <admin type="source">http://www.fomento.es/MFOM/LANG_CASTELLANO/DIRECCIONES_GENERALES/INSTITUTO_GEOGRAFICO/Astronomia/InvestermSecacion/astronomia/protoestrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c8"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Star_cluster#/media/File:M92_arp_750pix.jpg">Star_Cluster.jpg</xref> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A collection of stars formed together from the + same gas cloud and bound together by mutual gravitational + attraction.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>star cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Most star clusters are too far away and the + white dwarfs are too faint to be seen by ground-based telescopes, + but Hubble's powerful vision sees many of them.</descrip> + <admin type="source">http://hubblesite.org/newscenter/archive/releases/star%20cluster/2008/25/full/</admin> + </descripGrp> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un grupo de estrellas atraídas entre sí por su + gravedad mutua.</descrip> + <admin type="source">http://iopscience.iop.org/1538-3881/129/5/2281/pdf/1538-3881_129_5_2281.pdf</admin> + </descripGrp> + <termSec> + <term>cúmulo estelar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">“Es como encontrar un pez fuera del agua”, dice + Ed Churchwell, profesor de astronomía de la Universidad de + Wisconsin-Madison, quien con un equipo de científicos de UW-Madison, + de la Universidad de Wyoming, de la Universidad de Boston, del + Instituto de Ciencia Espacial de Boulder, Colorado, y del Centro de + Ciencia Spitzer descubrieron este inusual cúmulo estelar con la + ayuda del Telescopio Espacial Spitzer de la NASA. </descrip> + <admin type="source">http://www.astroseti.org/vernew.php?codigo=1117</admin> + </descripGrp> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Los cúmulos de estrellas se clasifican en dos + grupos: cúmulos abiertos, que no poseen forma definida, y cúmulos + globulares, que son esféricos o casi esféricos.</descrip> + <admin type="source">http://www.astromia.com/universo/cumulos.htm</admin> + </descripGrp> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c9"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Milky_Way#/media/File:ESO-VLT-Laser-phot-33a-07.jpg">Milky_Way.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <descripGrp> + <descrip type="definition">A band of faint light across the sky, visible to + the naked eye on a moonless night, consisting of stars and glowing gas + in the disk of our own Galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>Galaxy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">If merging is an important pathway to the + formation of massive stars, then it is expected that some + highluminosity IRAS sources in our Galaxy have brightened or faded + since the IRAS observations were made.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + </termSec> + <termSec> + <term>Milky Way</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <descripGrp> + <descrip type="definition">Una galaxia espiral en la que se encuentra el + Sistema Solar y, por ende, la Tierra.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Vía_Láctea</admin> + </descripGrp> + <termSec> + <term>Galaxia</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">La Vía Láctea, también llamada la Galaxia, es un + agrupamiento de estrellas con forma de disco, que incluye al Sol y a + su sistema solar.</descrip> + <admin type="source">www.todoelsistemasolar.com.ar/vlactea.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>Vía Láctea</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">La Via Láctea és una galaxia grande, espiral y + puede tener unos 100.000 millones de estrellas, entre ellas, el Sol. </descrip> + <admin type="source">http://www.astromia.com/universo/vialactea.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">La galaxia Vía Láctea es una galaxia espiral que + es nuestro hogar, al igual que el de otras 100 mil millones + estrellas. </descrip> + <admin type="source">http://www.windows.ucar.edu/tour/link=/the_universe/Milkyway.sp.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c10"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Star#/media/File:The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA%27s_Solar_Dynamics_Observatory_-_20100819.jpg">Star.jpg</xref> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A large, luminous ball of gas generating energy + internally by nuclear fusion.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">While the behavior of stars forming by accretion + is reasonably well understood,the consequences of merging have not + been fully investermSecated.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una enorme y densa bola de gas que genera fusión + nuclear, liberando así una gran cantidad de energía</descrip> + <admin type="source">spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</admin> + </descripGrp> + <termSec> + <term>estrella</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las estrellas son enormes aglomeraciones de gas, + principalmente Hidrogeno, cuya temperatura es tan alta debido a la + fusión de este elemento, que irradian luz a lo largo de todo el + espectro electromagnético. Poseen diferentes temperaturas que varían + desde los 2000 grados Celsius hasta los 50000.</descrip> + <admin type="source">http://www.astrosurf.com/astronosur/estrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c11"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Ultraviolet#/media/File:UV_LED_Fluoresence.jpg">UV_Radiation.jpg</xref> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The region of the electromagnetic spectrum + spanning the wavelength range from the Lymann limit at 91.2 nm to 350 + nm.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>UV radiation</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">UV radiation from stars and shocks likely + provide the minimum level of ionization required to couple these + fields strongly to the entangled medium.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">Ultraviolet (UV) radiation is part of the + electromagnetic spectrum emitted by the sun. </descrip> + <admin type="source">http://www.who.int/uv/en/</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">La radiación electromagnética cuya longitud de + onda está comprendida aproximadamente entre los 400 nm y los 15 + nm.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Radiaci%C3%B3n_UV</admin> + </descripGrp> + <termSec> + <term>radiación UV</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">Los usuarios de camas solares se someten a dosis + considerables de radiaciones UV artificiales para conseguir un + bronceado complementario al obtenido al tomar el sol.</descrip> + <admin type="source">http://copublications.greenfacts.org/es/camas-solares/</admin> + </descripGrp> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">La radiación ultravioleta se encuentra entre la + luz visible y los rayos X del espectro electromagnético.</descrip> + <admin type="source">http://www.windows.ucar.edu/tour/link=/physical_science/magnetism/em_ultraviolet.sp.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c12"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Magnetic_field#/media/File:VFPt_magnets_BHM.svg">Magnetic_Field.jpg</xref> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A region subject to the influence of magnetism + that is manifested by the mechanical forces that it exerts upon + electricity moving across it and upon the poles of magnets placed in + it.</descrip> + <admin type="source">Merriam-Webster2002</admin> + </descripGrp> + <termSec> + <term>magnetic field</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Detailed consideration of the merger process + will require numerical modeling in which the hydrodynamics, effects + of gravity,magnetic fields, and radiation are considered + carefully.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un campo de fuerza creado como consecuencia del + movimiento de cargas eléctricas, del flujo de la electricidad.</descrip> + <admin type="source">http://www.greenfacts.org/es/glosario/abc/campo-magnetico.htm</admin> + </descripGrp> + <termSec> + <term>campo magnético</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El campo magnético es producido por la corriente + eléctrica que circula por un conductor.</descrip> + <admin type="source">http://teleformacion.edu.aytolacoruna.es/FISICA/document/teoria/A_Franco/elecmagnet/magnetico/cMagnetico.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c13"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Blue_straggler#/media/File:Ngc6397_hst_blue_straggler.jpg">Blue_Straggler.jpg</xref> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A blue main-sequence star, usually found in a + globular or open cluster that appears to be slower in its evolution than + other stars of similar mass and luminosity in the same + cluster.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>blue straggler</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Numerical models of stellar collisions leading + to the formation of blue stragglers in globular clusters (Lombardi + et al. 2002, 2003; Fregeau et al. 2004) indicate that merger + products have radii up to 30 times larger than that of an equivalent + main-sequence star.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Estrellas que aparentan una edad menor que la del + sistema estelar al que pertenecen, si se supone que se formaron junto + con él.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Estrella_rezagada_azul</admin> + </descripGrp> + <termSec> + <term>estrella rezagada azul</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Las últimas observaciones de las “rezagadas + azules”, estrellas atípicas que aparentan ser más jóvenes que el + sistema estelar al que pertenecen, han proporcionado dos modelos + diferentes sobre su origen.</descrip> + <admin type="source">http://mundoastronomia.portalmundos.com/nuevas-pistas-sobre-el-origen-de-las-estrellas-rezagadas-azules/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c14"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The sudden collapse of a massive star when the + internal pressure pushing outwards falls so that it cannot balance the + weight of material pressing inward.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>gravitational collapse</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Stars form from the gravitational collapse of + turbulent molecular cloud cores (Elmegreen & Scalo 2004; Mac Low + & Klessen 2004).</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado final de la evolución de una estrella + de gran masa en el que la materia se comprime bajo la acción de su + propia atracción gravitatoria, con desprendimiento de grandes cantidades + de energía.</descrip> + <admin type="source">http://www.conocimientosweb.net/portal/term6172.html</admin> + </descripGrp> + <termSec> + <term>colapso gravitacional</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Esto sucede si la masa de un pedazo de la nube + excede cierto valor crítico, de modo tal que la fuerza de gravedad + vence definitivamente y el pedazo empieza a contraerse, aumentando + su densidad. Este proceso se llama colapso gravitacional. </descrip> + <admin type="source">http://bibliotecadigital.ilce.edu.mx/sites/ciencia/volumen1/ciencia2/06/html/sec_15.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c15"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Binary_star#/media/File:Algol_AB_movie_imaged_with_the_CHARA_interferometer_-_labeled.gif">Binary_Star.jpg</xref> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A pair of stars in orbit around each other, held + together by the graviational attraction between them.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>binary star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">These authors considered collision partners + having similar masses and concluded that such interactions can at + most account for a small fraction of the observed binary star + population in young clusters.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un sistema estelar compuesto de dos estrellas que + orbitan mutuamente alrededor de un centro de masas común.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Estrella_binaria</admin> + </descripGrp> + <termSec> + <term>estrella binaria</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">La explosión de una estrella binaria dentro de + una nebulosa planetaria ha sido capturado por un equipo dirigido por + investermSecadores del University College of London UCL - es un + acontecimiento que no ha sido presenciado hace más de 100 + años.</descrip> + <admin type="source">http://www.astroelche.es/blog/index.php?blog=2&title=astronomos-capturam-la-explosion-de-una-&more=1&c=1&tb=1&pb=1</admin> + </descripGrp> + </termSec> + <termSec> + <term>estrella doble</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Una estrella doble es una pareja de estrellas + que se mantienen unidas por la fuerza de la gravitación y giran en + torno a su centro común.</descrip> + <admin type="source">http://www.astromia.com/universo/dobles.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c16"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Initial_mass_function#/media/File:LH_95.jpg" + >Initial_Mass_Function.JPG</xref> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A mathematical description of the relative + frequncy with which stars of various masses are formed.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>initial mass function</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">La expresión numérica que determina el número de + estrellas con masa en un rango determinado.</descrip> + <admin type="source">Basado en http://laeff.cab.inta-csic.es/modules.php?op=modload&name=phpWiki&file=index&pagename=Research-Estrellas-IMF</admin> + </descripGrp> + <termSec> + <term>función inicial de masa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Estado evolutivo y función inicial de masa de + cúmulos jóvenes en la gran nube de Magallanes (estudio en el + ultravioleta).</descrip> + <admin type="source">http://dialnet.unirioja.es/servlet/tesis?codigo=11651</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c17"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Bally2005</term> + + + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c18"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Cambridge2007</term> + + + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c19"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Merriam-Webster2002</term> + + + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c20"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Oxford2007</term> + + + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c21"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Supernova#/media/File:SN1994D.jpg">Supernova.jpg</xref> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A catastrophic stellar explosion in which so much + energy is released that the supernova alone can outshine an entire + galaxy of billions of stars.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>supernova</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The supermassive object may be eventually + disrupted by an unusually violent supernova explosion (a hypernova) + soon after formation.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella que estalla y lanza a todo su + alrededor la mayor parte de su masa a altísimas velocidades.</descrip> + <admin type="source">http://www.astromia.com/glosario/supernova.htm</admin> + </descripGrp> + <termSec> + <term>supernova</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Un equipo de científicos británicos propone esta + semana en la revista Nature que la tenue supernova SN2008ha, + descubierta por una adolescente estadounidense en noviembre de 2008, + podría ser la explosión de una estrella masiva, en lugar de proceder + de una enana blanca como se planteaba hasta ahora.</descrip> + <admin type="source">http://www.plataformasinc.es/index.php/esl/Noticias/Una-supernova-observada-por-astronomos-aficionados-abre-el-debate-entre-los-profesionales</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c22"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>Moore2003</term> + + + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c23"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Red_giant#/media/File:Mira_1997.jpg">Red_Giant.jpg</xref> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cool, large and highly luminous star that has + left the main sequence and is powered by heavier elements than + hydrogen.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>red giant</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The core temperature becomes so high that helium + start to 'burn', producing carbon; around this active core there is + a shell where hydrogen is still producing energy. The star becomes + unstable, and the outer layers swell out, cooling as they do so. The + star becomes a red giant.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella de masa baja o intermedia (menos de + 8-9 masas solares) que, tras haber consumido el hidrógeno en su núcleo + durante la etapa de secuencia principal, convirtiéndolo en helio por + fusión nuclear, comienza a quemar hidrógeno en una cáscara alrededor del + núcleo de helio inerte.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Gigante_roja</admin> + </descripGrp> + <termSec> + <term>gigante roja</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">La gigante roja S Orionis (S Ori) es una + estrella variable del tipo Mira. Su masa es similar a la del Sol, + con la diferencia de que está mucho más cerca de convertirse en una + enana blanca, el mismo final que le espera a nuestro Sol dentro de 5 + mil millones de años.</descrip> + <admin type="source">http://www.solociencia.com/astronomia/07071709.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c24"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Red_dwarf#/media/File:New_shot_of_Proxima_Centauri,_our_nearest_neighbour.jpg">Red_Dwarf.jpg</xref> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cool, faint, low-mass star lying at the lower + end of the main sequence of spectral type K or M.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>red dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The dim red dward Proxima, more than a degree + away from Alpha, is slightly closer to us.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella pequeña y relativamente fría de la + secuencia principal, ya sea de tipo espectral K tardío o M.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Enana_roja</admin> + </descripGrp> + <termSec> + <term>enana roja</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El planeta que se ha descubierto girando + alrededor de esta enana roja tiene una masa equivalente a la de + Neptuno, es decir, es sólo 17 veces mayor que la Tierra y mucho + menor que Saturno.</descrip> + <admin type="source">http://axxon.com.ar/not/157/c-1570034.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c25"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Stellar_classification#/media/File:Zeta_Puppis.png">Spectral_Type.jpg</xref> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A means of classifying stars according to the + details of their spectrum, depending largely on their surface + temperature.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>spectral type</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">In this version of a typical HR diagram, the + stars are plotted according to their spectral types and suface + temperatures (horzontal axis, x) and their luminositites in therms + of the Sun (vertical axis, y).</descrip> + <admin type="source">Moore2003, 171</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El espectro de una estrella clasificado por una + letra (O, B, A, F, G, K, M, R, N, S) seguida de un digito que describe + el color de la estrella y su temperatura.</descrip> + <admin type="source">Basado en http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Tipo_espectral.html</admin> + </descripGrp> + <termSec> + <term>tipo espectral</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En el gráfico superior se muestra la intensidad + de las líneas espectrales según la temperatura de la estrella (tipo + espectral)</descrip> + <admin type="source">http://www.astrosurf.com/astronosur/estrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c26"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/White_dwarf#/media/File:Sirius_A_and_B_Hubble_photo.editted.PNG">White_Dwarf.jpg</xref> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A small dense star that is has run out of fuel + for nuclear fusion, collapsing under its own gravity and blowing off its + outer layers to form a planetary nebula in the process.</descrip> + <admin type="source">Based on Oxford2007 and Cambridge2007</admin> + </descripGrp> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">To the upper right lie giants and supergiants of + tremendous luminosity, while to the lower left there are the white + dwarfs, which are in a differnt category and were not known when HR + Diagrams were introduced.</descrip> + <admin type="source">Moore2003, 170</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un remanente estelar que se genera cuando una + estrella de masa menor a 9-10 masas solares ha agotado su combustible + nuclear.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Enana_blanca</admin> + </descripGrp> + <termSec> + <term>enana blanca</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Cuando el material fusionable se agota la + estrella pierde la presión interna producida por la fusión nuclear y + puede colapsar inmediatamente terminando en una enana + blanca.</descrip> + <admin type="source">http://astroverada.com/_/Main/T_evolucion.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c27"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Planetary_nebula#/media/File:NGC6543.jpg">Planetary_Nebula.jpg</xref> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A bright cloud of glowing gas and dust + surrounding a highly evolved star.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The star's outer layers are thrown off, and for + a cosmically brief period - no more than about 100,000 years - we + have the phenomenon of what is termed a planetary nebula.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una nebulosa de emisión consistente en una + envoltura brillante en expansión de plasma y gas ionizado, expulsada + durante la fase de rama asintótica gigante que atraviesan las estrellas + gigantes rojas en los últimos momentos de sus vidas.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Nebulosa_planetaria</admin> + </descripGrp> + <termSec> + <term>nebulosa planetaria</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las nebulosas planetarias resultan objetos muy + espectaculares si se observan con un telescopio de media o gran + potencia.</descrip> + <admin type="source">http://www.astromia.com/glosario/nebulosaplanetaria.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c28"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Emission_nebula#/media/File:Ring_Nebula.jpg">Emission_Nebula.jpg</xref> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A luminous cloud of gas and sust in space which + shines with its own light, which can be generated in several + ways.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">In this and other similar emission nebulae, + energetic ultraviolet light from a hot young star strips electrons + from the surrounding hydrogen atoms.</descrip> + <admin type="source">http://apod.nasa.gov/apod/emission_nebulae.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una nube de gas interestelar que brilla por la + excitación del gas, causado por radiación ultravioleta emitida por + estrellas inmersas en la nube o por calentamiento debido a otro + mecanismos. </descrip> + <admin type="source">http://www.diclib.com/Nebulosa%20de%20emisi%C3%B3n/show/en/es_astronomia/726</admin> + </descripGrp> + <termSec> + <term>nebulosa de emisión</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las nebulosas de emisión estan normalmente en + los lugares de formación de estrellas.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c29"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Nebula#/media/File:Eagle_nebula_pillars.jpg">Nebula.jpg</xref> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cloud of interstellar gas and dust.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: singular</note> + <descripGrp> + <descrip type="context">According to current theory, a star begins by + condensing out of the tenuous material making up a nebula.</descrip> + <admin type="source">Moore2003, 172</admin> + </descripGrp> + </termSec> + <termSec> + <term>nebulae</term> + + + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: plural</note> + <descripGrp> + <descrip type="context">Other nebulae are within the range of small + telescopes.</descrip> + <admin type="source">Moore2003, 187</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Regiones del medio interestelar constituidas por + gases (principalmente hidrógeno y helio) y polvo.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Nebulosa</admin> + </descripGrp> + <termSec> + <term>nebulosa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">A unos 1.500 años-luz de distancia, dentro de + nuestro brazo espiral en la Vía Láctea, la Nebulosa de Orión está en + el centro de la región de la Espada de la constelación de Orión el + Cazador, que domina el cielo nocturno a inicios del invierno, en las + latitudes Norte.</descrip> + <admin type="source">http://www.oarval.org/OrionNebsp.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c30"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Dark_nebula#/media/File:All_Quiet_in_the_Nursery%3F.jpg">Dark_Nebula.jpg</xref> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A type of interstellar cloud that is so dense + that it obscures the light from the background emission or reflection + nebula or that it blocks out background stars.</descrip> + <admin type="source">http://en.wikipedia.org/wiki/Dark_nebula</admin> + </descripGrp> + <termSec> + <term>dark nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">There is no difference between a dark nebula and + a bright one, except for the lack of illumination.</descrip> + <admin type="source">Moore2003, 187</admin> + </descripGrp> + </termSec> + <termSec> + <term>absorbtion nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">An absorption nebula is a dense cloud of dust + and gas. From the point of view of an observer on Earth, it absorbs + the light from more distant stars, creating a dark, starless + region.</descrip> + <admin type="source">http://www.glyphweb.com/esky/concepts/absorptionnebula.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Nubes de polvo que simplemente tapan la luz de lo + que haya detras.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + <termSec> + <term>nebulosa oscura</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Aqui hay un mapa que muestra las regiones de + nebulosas oscuras que estan en un radio de 2000 años luz.</descrip> + <admin type="source">http://www.atlasoftheuniverse.com/espanol/darknebs.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">El caso más opuesto a las nebulosas de emisión + son las nebulosas de absorción (nebulosas oscuras). Estas ni si + quiera están rodeadas de estrellas lo suficientemente potentes ni + cercanas para hacer llegar la luminosidad suficiente para que la + nebulosa pueda reflejarla.</descrip> + <admin type="source">http://www.blogdeastronomia.es/astronomia/formacion-de-estrellas/las-nebulosas</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c31"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Reflection_nebula#/media/File:Reflection.nebula.arp.750pix.jpg">Reflection_Nebula.jpeg</xref> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cloud of interstellar gas and dust that appears + bight because it reflects or scatters starlight.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>reflection nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Just weeks after NASA astronauts repaired the + Hubble Space Telescope in December 1999, the Hubble Heritage Project + snapped this picture of NGC 1999, a reflection nebula in the + constellation Orion. </descrip> + <admin type="source">http://www.nasa.gov/multimedia/imagegallery/image_feature_701.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Nubes de polvo que simplemente reflejan la luz de + una estrella o estrellas cercanas.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + <termSec> + <term>nebulosa de reflexión</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Como el propio nombre implica, esta nebulosa de + reflexión asociada con la estrella Rigel, se asemeja a una vieja + arpía de un cuento de hadas. </descrip> + <admin type="source">http://www.astrofotos.com.es/2008/11/nebulosa-de-la-cabeza-de-bruja.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c32"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Neutron_star#/media/File:PIA18848-PSRB1509-58-ChandraXRay-WiseIR-20141023.jpg">Neutron_Star.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">After its Main Sequence period the star becomes + a red supergiant and may explode as a supernova. It may end as a + neutron star or pulsar, although if its mass is even greater it may + poroduce a black hole.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <descripGrp> + <descrip type="definition">Un cuerpo pequeño muy denso que se forma en el + envejecimiento de una estrella pesada y que está formada únicamente por + partículas subatómicas denominadas neutrones.</descrip> + <admin type="source">http://www.astroasa.com.ar/diccionario_astro.htm</admin> + </descripGrp> + <termSec> + <term>estrella de neutrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El Gran Telescopio Canarias (GTC), instalado en + el Observatorio del Roque de los Muchachos (La Palma), ha obtenido + imágenes de una profundidad "sin precedentes" de una estrella de + neutrones del tipo magnetar, de las que se conocen seis, según ha + informado el Instituto de Astrofísica de Canarias (IAC).</descrip> + <admin type="source">http://www.rtve.es/noticias/20100301/imagen-unica-estrella-neutrones-cazada-canarias/321412.shtml</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c33"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The maximum possible mass of a degenerate star, + above which it will be unable to support itself against the inward pull + of its own gravity. </descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">However, there is a limit, once the mass of the + white dwarf becomes greater than 1.4 time that of the sun )a value + known as the Chandrasekhar limit, after the Indian astronomer who + first worked it out=, the carbon detonates, and in a matter of a few + seconds the white dwarf blows itself to pieces.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El límite de masa más allá del cual la + degeneración de electrones no es capaz de contrarrestar la fuerza de + gravedad en un remanente estelar, produciéndose un colapso que origina + una estrella de neutrones o un agujero negro. </descrip> + <admin type="source">http://es.wikipedia.org/wiki/L%C3%ADmite_de_Chandrasekhar</admin> + </descripGrp> + <termSec> + <term>límite de Chandrasekhar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Descubrió una masa (aproximadamente 1.5 veces la + masa del Sol) en la que una estrella fría no podría soportar su + gravedad. Esto es lo que se conoce como el límite de + Chandrasekhar.</descrip> + <admin type="source">http://html.rincondelvago.com/agujeros-negros_5.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c34"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The state of degeneracy attained when the density + of matter is so high that neutrons cannot be packed any more closely + together.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado de degeneración alcanzado cuando la + densidad de materia es tan alta, que los neutrones no pueden juntarse + más.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>degeneración de neutrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c35"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The radius of the event horizon of a black + hole.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>Schwarzschild radius</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The critical radius of a non-rotating black hole + is called the Schwarzschild radius, after the German astronomer who + investermSecated the problem mathematically as long ago as 1916: the + boundary around the collapsed star having this radius is termed the + 'event horizon'.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El radio del horizonte de sucesos para un agujero + negro.</descrip> + <admin type="source">http://www.astrocosmo.cl/glosario/glosar-r.htm</admin> + </descripGrp> + <termSec> + <term>radio de Schwarzschild</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Me pareció muy interesante este vídeo del + proyecto Sixty Symbols de la Universidad de Nottingham en el que + explican de forma divulgativa qué es el radio de Schwarzschild. + Básicamente es el radio de un agujero negro.</descrip> + <admin type="source">http://www.microsiervos.com/archivo/ciencia/agujeros-negros-y-el-radio-de-schwarzschild.html</admin> + </descripGrp> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c36"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The surface of a black hole.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>event horizon</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Narayan and Heyl have calculated that if very + heavy objects do not collapse to a point with an event horizon but + instead have a surface, they would eject as many type 1 bursts as + neutron stars.</descrip> + <admin type="source">http://www.newscientist.com/article/dn2527-astronomers-reach-the-event-horizon.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El superficie de un agujero negro.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>horizonte de sucesos</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En consecuencia, aquí, cuando nos estamos + refiriendo a una «singularidad», estamos pensando en una masa con + volumen nulo rodeada de una frontera gravitacional llamada + «horizonte de sucesos», de la cual nada puede escapar. </descrip> + <admin type="source">http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>horizonte de eventos</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">InvestermSecadores de la Universidad de St. Andrews + en Escocia, afirman haber encontrado una forma de simular un + horizonte de eventos de un agujero negro – no a través de una nueva + técnica de observación cósmica, ni mediante una supercomputadora de + alta potencia … sino en el laboratorio.</descrip> + <admin type="source">http://www.cienciakanija.com/2008/02/14/horizonte-de-eventos-sintetico-de-un-agujero-negro-creado-en-un-laboratorio-del-reino-unido/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c37"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Proton%E2%80%93proton_chain_reaction#/media/File:Fusion_in_the_Sun.svg">PP_Chain.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>proton-proton chain reaction</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">The proton–proton chain reaction is one of + several fusion reactions by which stars convert hydrogen to helium, + the primary alternative being the CNO cycle. The proton–proton chain + dominates in stars the size of the Sun or smaller.</descrip> + <admin type="source">http://www.absoluteastronomy.com/topics/Proton-proton_chain_reaction</admin> + </descripGrp> + </termSec> + <termSec> + <term>PP chain</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">The primary reactions in the main branch of the + PP chain are illustrated in the following figure.</descrip> + <admin type="source">http://csep10.phys.utk.edu/astr162/lect/energy/ppchain.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>proton-proton reaction</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The gamma rays produced in the proton-proton + reaction take one to 10 million years to work their way out from the + star's core, being scattered numerous times and losing energy as + they go, until they emerge from the surface as rays of light and + heat. Inside the Sun, about 655 million tons of hydrogen are + converted into 650 million tons of helium every second. In stars + heavier than about 2 solar masses, in which the core temperature is + more than about 18 million K, the dominant process in which energy + is produced by the fusion of hydrogen into helium is a different + reaction chain known as the carbon-nitrogen cycle. </descrip> + <admin type="source">http://www.daviddarling.info/encyclopedia/P/proton-proton_chain.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un conjunto de procesos nucleares mediante los + cuales cuatro núcleos de átomos de hidrógeno se combinan para formar uno + de helio, produciendo gran cantidad de energía.</descrip> + <admin type="source">http://www.avizora.com/publicaciones/astronomia/textos/glosario_astronomia_afines_0006.htm</admin> + </descripGrp> + <termSec> + <term>cadena protón-protón</term> + + + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c38"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/CNO_cycle#/media/File:CNO_cycle.png">CNO_Cycle.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>carbon-nitrogen cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The Helium burning process are important 1) + Carbon-Nitrogen cycle at which a carbon-12 nucleus (12C) capture + proton and is converted into 13C, Nitrogen-4 and nitrogen –15. </descrip> + <admin type="source">http://www.sciencenews.org/view/generic/id/44769/title/Supernova_may_be_in_a_new_class</admin> + </descripGrp> + </termSec> + <termSec> + <term>CNO cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</descrip> + <admin type="source">http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</descrip> + <admin type="source">http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Dr. von Weizsäcker is best known in science for + what is sometimes called the Bethe-Weizsäcker cycle, proposed by him + and the physicist Hans Bethe in the late 1930s as the nuclear + reactive process by which energy is generated in stars. </descrip> + <admin type="source">http://www.nytimes.com/2007/05/02/world/europe/02weizsacker.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>carbon cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The main theme of the carbon cycle is the adding + of protons, but after a carbon-12 nucleus fuses with a proton to + form nitrogen-13, one of the protons decays with the emission of a + positron and a neutrino to form carbon -13.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/carbcyc.html</admin> + </descripGrp> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">We argue that it may be possible to exploit + neutrinos from the CN cycle and p-p chain to determine the + primordial solar core abundances of C and N at an interesting level + of precision.</descrip> + <admin type="source">http://iopscience.iop.org/0004-637X/687/1/678</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>ciclo CNO</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">Existen dos formas fundamentales en las que una + estrella fusiona hidrógeno para producir helio: la cadena + protón-protón y el ciclo CNO.</descrip> + <admin type="source">http://eltamiz.com/2007/09/06/la-vida-privada-de-las-estrellas-las-entranas-de-una-estrella/</admin> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">No se pretende copiar los complicados ciclos de + reacciones que se dan en el interior de las estrellas, como la + cadena protón-protón o el ciclo del carbono-nitrógeno-oxígeno (esta + última más importante en las estrellas más masivas que el Sol). </descrip> + <admin type="source">http://www.zaragoza.es/ciudad/conocimiento/zivis/aplicaciones.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">El ciclo del carbono comienza y acaba con un + núcleo de carbono 12 que actúa como catalizador en la producción de + un núcleo de helio a partir de núcleos de hidrógeno; también se + producen neutrinos y rayos gamma. </descrip> + <admin type="source">http://www.astromia.com/glosario/ciclocno.htm</admin> + </descripGrp> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">En las estrellas de gran masa, que queman su + hidrógeno mucho más rápidamente, predomina el ciclo del + carbono-nitrógeno (CN).</descrip> + <admin type="source">http://www.aavbae.net/bol17/evolucion.php</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c39"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A state of matter attained when atomic particles + are packed together as termSechtly as is physically possible, at densities + of several thousand tonnes per cubic metre.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Although Eddington raised doubts at the meeting + about the concept of relativistic degeneracy, astronomy has since + found that all white dwarfs for which masses have been measured fall + neatly below the Chandrasekhar limit without exception. Today there + are no doubts about his work on degeneracy. </descrip> + <admin type="source">http://www.tamil.net/people/andrew/subra.htm</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Estado de la materia producido cuando las + partículas atómicas tienen el mayor empaquetamiento físicamente posible, + con densidades de varios miles de toneladas por centímetro cúbico. </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + <termSec> + <term>degeneración</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Estas estrellas son aún más densas que las + enanas blancas, y más pequeñas. Se mantienen por un proceso de + "degeneración de neutrones" o "repulsión de neutrones".</descrip> + <admin type="source">http://www.austrinus.com/index.php?option=com_content&view=article&id=157&Itemid=112</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c40"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>Oxford2003</term> + + + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c41"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The state of degeneracy attained when the density + of matter is so high that electrons cannot be packed any closer + together.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado de degeneración alcanzado cuando la + densidad de materia es tan grande, que los electrones no pueden + empaquetarse más.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>degeneración de electrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + </termSec> + <termSec> + <term>degeneración electrónica</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Las fuerzas gravitatorias actuantes en un cuerpo + celeste masivo pueden comprimir su materia hasta un estado de + degeneración electrónica y no más, ya que el principio de exclusión + impide a dos electrones ocupar el mismo nivel de energía. </descrip> + <admin type="source">http://www.portalplanetasedna.com.ar/estrella2.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c42"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A mathematical point at which certain physical + quantities reach infinite values.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>singularity</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">A singularity means a point where some property + is infinite. For example, at the center of a black hole, according + to classical theory, the density is infinite (because a finite mass + is compressed to a zero volume). Hence it is a singularity. </descrip> + <admin type="source">http://curious.astro.cornell.edu/question.php?number=55</admin> + </descripGrp> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un punto matemático en el que ciertas cantidades + físicas alcanzan valores infinitos.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>singularidad</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las singularidades ocurren en el Big Bang, en + los agujeros negros y en el Big Crunch (que podría ser considerado + como una unión de agujeros negros).</descrip> + <admin type="source">http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</admin> + </descripGrp> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c43"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Solar_mass#/media/File:Rho_Cassiopeiae_Sol_VY_Canis_Majoris.png">Solar_Mass.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A unit of mass used in stellar and galactic + astronomy, equivalent to the mass of the sun, 1.989 x 10^30 + kg.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>solar mass</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">This page now explores the fate of stars of 8 + solar masses or less.</descrip> + <admin type="source">http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_deathlow.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una unidad de medida utilizada en astronomía y + astrofísica para medir comparativamente la masa de las estrellas y otros + objetos astronómicos muy masivos como galaxias.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Masa_solar</admin> + </descripGrp> + <termSec> + <term>masa solar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Para una nube con la masa de nuestro Sol, el + colapso dura unos 10 millones de años, mientras que si su masa fuese + mucho más pequeña, por ejemplo un décimo de la masa solar, este + proceso podría durar hasta 800 millones de años.</descrip> + <admin type="source">http://www.tayabeixo.org/sist_solar/hipotesis/formacion_sistsolar.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c44"> + <descrip type="subjectField">General</descrip> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Triple-alpha_process#/media/File:Triple-Alpha_Process.svg" + >Triple-Alpha_Process.jpg</xref> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The chain of nuclear reactions by which carbon is + synthesized in the interiors of stars through the fusion of three helium + nuclei(alpha particles).</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>triple-alpha process</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">This small concentration of Be-8 can begin to + undergo reactions with other He-4 nuclei to produce an excited state + of the mass-12 isotope of Carbon. This excited state is unstable, + but a few of these excited Carbon nuclei emit a gamma-ray quickly + enough to become stable before they disintegrate. This extremely + improbable sequence is called the triple-alpha process because the + net effect is to combine 3 alpha particles (that is, 3 He-4 nuclei) + to form a C-12 nucleus. </descrip> + <admin type="source">http://csep10.phys.utk.edu/astr162/lect/energy/triplealph.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El proceso por el cual tres núcleos de helio + (partículas alfa) se transforman en un núcleo de carbono.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Proceso_triple-alfa</admin> + </descripGrp> + <termSec> + <term>proceso triple-alfa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">También debe tenerse en cuenta una tercera + reacción de gran importancia, denominada proceso triple + alfa.</descrip> + <admin type="source">http://feinstein.com.ar/Composicion.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c45"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Black_dwarf#/media/File:Black_dwarf.jpg">Black_Dwarf.jpg</xref> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A degenerate star that has cooled until it is no + longer visible.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>black dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Banprupt though it is, a white swarf still has a + high surface temperature when it is first formed; up to 100,000 + degrees C in some cases and it continues to radiate. Gradually it + fades, and must end up as a cold, dead black dwarf; but at the + moment no white dwarf with a surface temperature of below 3,000 + degrees C has been found, and it may be that the universe is not yet + old enough for any black dwarfs to have been formed.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella creada cuando una enana blanca se + enfría lo suficiente como para dejar de emitir calor o luz en cantidad + significativa.</descrip> + <admin type="source">http://spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</admin> + </descripGrp> + <termSec> + <term>enana negra</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">No se conoce, todavía, la cantidad de Enanas + Negras que pueblan en realidad nuestro Universo. El tiempo estimado + para que una Enana Blanca se enfríe lo suficiente para volverse + Negra, se estima entre diez y cien mil millones de años, y nuestro + Universo no es aún lo bastante viejo, nada más que para que existan + algunas enanas blancas que se han enfriado lo suficiente para + alcanzar la etapa de enanas negras.</descrip> + <admin type="source">http://celestia.albacete.org/celestia/celestia/stars/enana12.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> + +</tbx> diff --git a/spec/fixtures/TBX_test_files/basic_good.tbx b/spec/fixtures/TBX_test_files/basic_good.tbx new file mode 100644 index 0000000..20ca7eb --- /dev/null +++ b/spec/fixtures/TBX_test_files/basic_good.tbx @@ -0,0 +1,4028 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../schematrons/basic_schema.sch" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?> +<?xml-model href="../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<tbx type="TBX-Basic" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + + <text> + <body> + <conceptEntry id="c1"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Galaxy_cluster#/media/File:Galaxy_cluster_IDCS_J1426.jpg">Open_Cluster.JPG</xref> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A group of stars formed together in the spiral + arms of a galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>open cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Over 1100 open clusters are known in our Milky + Way Galaxy, and this is probably only a small percentage of the + total population which is probably some factor higher; estimates of + as many as about 100,000 Milky Way open clusters have been given. </descrip> + <admin type="source">http://seds.org/MESSIER/open.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>galactic cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <descripGrp> + <descrip type="context">In contrast, the galactic cluster represented by + M29 is a grouping of stars—a “knot” of stars in the stellar + backdrop.</descrip> + <admin type="source">http://www.eastbayastro.org/2000/0900/r0900-8.htm</admin> + </descripGrp> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una acumulación de una docena hasta varios miles + de jóvenes estrellas en el plano de las galaxias.</descrip> + <admin type="source">http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Cumulo_abierto.html</admin> + </descripGrp> + <termSec> + <term>cúmulo abierto</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">M7 es uno de los cúmulos abiertos estelares más + prominentes del cielo. El cúmulo, dominado por brillantes estrellas + azules, puede ser visto a ojo desnudo en un cielo oscuro en la cola + de la constelación del Escorpión (Scorpius).Contiene unas 100 + estrellas en total, tiene una edad aproximada de 200 millones de + años, mide 25 años luz de ancho, y se encuentra a unos 1000 años luz + de distancia.</descrip> + <admin type="source">http://observatorio.info/2009/11/m7-cumulo-abierto-en-scorpius-2/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c2"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Accretion_disk#/media/File:Star_with_accretion_disk.jpg">Accretion_Disk.jpg</xref> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A structure that forms around a compact object + (e.g. a white dwarf, neutron star, or black hole) when matter flows + towards it.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>circumstellar accretion disk</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">In contrast with the violence of merging, the + gradual growth of massive stars by accretion is likely to produce + less infrared variability, relatively thin circumstellar accretion + disks that maintain their orientation, and collimated bipolar + outflows that are scaled-up versions of those produced by low-mass + young stellar objects.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>accretion disc</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Accretion Disc Evolution in Single and Binary T + Tauri Stars</descrip> + <admin type="source">http://cdsweb.cern.ch/record/369655</admin> + </descripGrp> + </termSec> + <termSec> + <term>circumstellar disk</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Our results suggest a scenario of a central star + accreting material from a circumstellar disc at the centre of a cool + extended rotating torus, while driving a fast bipolar wind. </descrip> + <admin type="source">http://adsabs.harvard.edu/abs/2010MNRAS.402.1504D</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estructura en forma de disco alrededor de un + objeto central masivo que alimenta el cuerpo central siendo atraido por + éste y contribuye a su aumento de masa.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Disco_de_acreci%C3%B3n</admin> + </descripGrp> + <termSec> + <term>disco de acreción</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Lo que alimenta esta actividad es el gas + extraído de la estrella normal, que, cayendo en espiral hacia el + agujero negro, se acumula en un denso disco de acreción.</descrip> + <admin type="source">http://www.amazings.com/ciencia/noticias/010210e.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Imágenes de estrellas jóvenes con discos de + acrecimeinto y chorros colimados de material, tomadas con el + telescopio espacial Hubble.</descrip> + <admin type="source">http://www.laeff.inta.es/index.php?op=modload&name=phpWiki&file=index&pagename=Research-Brown%20Dwarfs-BD_esp-DiscosAcrecimiento</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c3"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Black_hole#/media/File:BH_LMC.png">Black_Hole.jpg</xref> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A region of space where the gravitational force + is so strong that not even light can escape from it.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>black hole</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">As matter spirals toward and into the black + hole, some of its gravitational potential energy may be efficiently + converted into relativistic jets launched by the magnetic field + along the spin axis.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un punto super-denso en el espacio formado por el + colapso de una estrella donde nada puede escapar de su influencia + gravitacional. </descrip> + <admin type="source">www.atlasoftheuniverse.com/espanol/glossary.html</admin> + </descripGrp> + <termSec> + <term>agujero negro</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En teoría un agujero negro se origina hacia el + final de la vida de una estrella, cuando ésta se contrae mas allá de + un límite determinado - conocido como radio de Schwarzschild - y se + hace más pequeña y mas densa que una estrella de neutrones, tanto + que ni la luz puede escapar de su campo gravitatorio.</descrip> + <admin type="source">http://html.rincondelvago.com/agujeros-negros_5.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c4"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Gamma-ray_burst#/media/File:GRB080319B_illustration_NASA.jpg">Gamma_Ray_Burst.jpg</xref> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A temporary intese burst of gamma rays and X-rays + from a cosmic source.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>gamma-ray burst</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>GRB</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">acronym</termNote> + <descripGrp> + <descrip type="context">The off-axis collisions and merging of stars + near the top of the stellar mass spectrum may result in the + production of GRBs.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Destellos de rayos gamma que pueden durar desde + unos nanosegundos hasta cerca de una hora.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Brote_de_rayos_gamma</admin> + </descripGrp> + <termSec> + <term>explosión de rayos gamma</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Una poderosa explosión de rayos gamma, detectada + el 19 de marzo por el satélite Swift, de la NASA, batió el récord + como el objeto más distante que se pudo observar a simple + vista.</descrip> + <admin type="source">http://ciencia.nasa.gov/headlines/y2008/21mar_nakedeye.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">John Ellis (entrevistado por Punset en su + despacho en el CERN en un programa de Redes) y sus colaboradores + mostraron cómo utilizar las propiedades de los grandes brotes de + rayos gamma (gamma-ray bursters o GRBs) para responder a esta + cuestión.</descrip> + <admin type="source">http://francisthemulenews.wordpress.com/2009/02/21/el-mayor-brote-de-rayos-gamma-grb-080916c-acerca-la-gravedad-cuantica-al-mundo-de-planck/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c5"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Globular_cluster#/media/File:A_Swarm_of_Ancient_Stars_-_GPN-2000-000930.jpg">Globular_Cluster.jpg</xref> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A roughly spherical group of old stars in the + halo of the galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>globular cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Although the standard accretion scenario may + well explain the formation of most massive stars, the existence of + blue stragglers in globular clusters indicates that mergers do occur + in nature.</descrip> + <admin type="source">Birth of High-Mass Stars</admin> + </descripGrp> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un tipo de cúmulo estelar que consiste en una + agrupación de miles de estrellas viejas, gravitacionalmente ligadas, con + distribución aproximadamente esférica, y que orbita en torno a una + galaxia de manera similar a un satélite.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/C%C3%BAmulo_globular</admin> + </descripGrp> + <termSec> + <term>cúmulo globular</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context"> De los 200 cúmulos globulares que sobreviven + hoy, M3 es uno de los más grande y luminoso, fácilmente observable + con binoculares en el hemisferio Norte del cielo.</descrip> + <admin type="source">http://www.tayabeixo.org/portadas/m3.htm</admin> + </descripGrp> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c6"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Main_sequence#/media/File:HRDiagram.png">Main_Sequence.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <descripGrp> + <descrip type="definition">Of or dealing with a major group of stars forming + a band stretching from upper left to lower right on a + Hertzsprung-Russell diagram when being plotted by luminosity and surface + temperature.</descrip> + <admin type="source">http://en.wiktionary.org/wiki/main-sequence</admin> + </descripGrp> + <termSec> + <term>main-sequence</term> + + + <termNote type="partOfSpeech">adjective</termNote> + <descripGrp> + <descrip type="context">However, immediately after its formation, the + merger product is likely to have a photospheric radius considerably + larger than that of a main-sequence star with the same + mass.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Pertenece a las estrellas en la región del + diagrama de Hertzsprung-Russell en la que se encuentran la mayor parte + de las estrellas que transforman hidrógeno en helio.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Secuencia_principal</admin> + </descripGrp> + <termSec> + <term>de secuencia principal</term> + + + <termNote type="partOfSpeech">adjective</termNote> + <descripGrp> + <descrip type="context">Por ejemplo, nuestro sol es una estrella de + secuencia principal regular de tamaño pequeño. </descrip> + <admin type="source">http://celestia.albacete.org/celestia/celestia/stars/secu5.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c7"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Protostar#/media/File:A_diamond_in_the_dust.jpg">Protostar.JPG</xref> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A star in the earliest observable stage of + formation.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>protostar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Alternatively, it has been suggested that + massive stars form from the merging of lower mass protostars in + high-density protostar clusters (Bonnell et al.1998; Stahler et al. + 2000; Bonnell 2002; Zinnecker & Bate 2002).</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <descripGrp> + <descrip type="definition">Una región muy densa o descorazonada de nubes + moleculares donde existen estrellas en proceso de formación.</descrip> + <admin type="source">www.astrocosmo.cl/glosario/glosar-p.htm</admin> + </descripGrp> + <termSec> + <term>protoestrella</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En estos primeros estadios, la protoestrella es + un objeto muy activo, y produce un viento bipolar formado por dos + chorros opuestos de material de alta velocidad. </descrip> + <admin type="source">http://www.fomento.es/MFOM/LANG_CASTELLANO/DIRECCIONES_GENERALES/INSTITUTO_GEOGRAFICO/Astronomia/InvestermSecacion/astronomia/protoestrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c8"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Star_cluster#/media/File:M92_arp_750pix.jpg">Star_Cluster.jpg</xref> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A collection of stars formed together from the + same gas cloud and bound together by mutual gravitational + attraction.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>star cluster</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Most star clusters are too far away and the + white dwarfs are too faint to be seen by ground-based telescopes, + but Hubble's powerful vision sees many of them.</descrip> + <admin type="source">http://hubblesite.org/newscenter/archive/releases/star%20cluster/2008/25/full/</admin> + </descripGrp> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un grupo de estrellas atraídas entre sí por su + gravedad mutua.</descrip> + <admin type="source">http://iopscience.iop.org/1538-3881/129/5/2281/pdf/1538-3881_129_5_2281.pdf</admin> + </descripGrp> + <termSec> + <term>cúmulo estelar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">“Es como encontrar un pez fuera del agua”, dice + Ed Churchwell, profesor de astronomía de la Universidad de + Wisconsin-Madison, quien con un equipo de científicos de UW-Madison, + de la Universidad de Wyoming, de la Universidad de Boston, del + Instituto de Ciencia Espacial de Boulder, Colorado, y del Centro de + Ciencia Spitzer descubrieron este inusual cúmulo estelar con la + ayuda del Telescopio Espacial Spitzer de la NASA. </descrip> + <admin type="source">http://www.astroseti.org/vernew.php?codigo=1117</admin> + </descripGrp> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Los cúmulos de estrellas se clasifican en dos + grupos: cúmulos abiertos, que no poseen forma definida, y cúmulos + globulares, que son esféricos o casi esféricos.</descrip> + <admin type="source">http://www.astromia.com/universo/cumulos.htm</admin> + </descripGrp> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c9"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Milky_Way#/media/File:ESO-VLT-Laser-phot-33a-07.jpg">Milky_Way.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <descripGrp> + <descrip type="definition">A band of faint light across the sky, visible to + the naked eye on a moonless night, consisting of stars and glowing gas + in the disk of our own Galaxy.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>Galaxy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">If merging is an important pathway to the + formation of massive stars, then it is expected that some + highluminosity IRAS sources in our Galaxy have brightened or faded + since the IRAS observations were made.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + </termSec> + <termSec> + <term>Milky Way</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <descripGrp> + <descrip type="definition">Una galaxia espiral en la que se encuentra el + Sistema Solar y, por ende, la Tierra.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Vía_Láctea</admin> + </descripGrp> + <termSec> + <term>Galaxia</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">La Vía Láctea, también llamada la Galaxia, es un + agrupamiento de estrellas con forma de disco, que incluye al Sol y a + su sistema solar.</descrip> + <admin type="source">www.todoelsistemasolar.com.ar/vlactea.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>Vía Láctea</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">La Via Láctea és una galaxia grande, espiral y + puede tener unos 100.000 millones de estrellas, entre ellas, el Sol. </descrip> + <admin type="source">http://www.astromia.com/universo/vialactea.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">La galaxia Vía Láctea es una galaxia espiral que + es nuestro hogar, al igual que el de otras 100 mil millones + estrellas. </descrip> + <admin type="source">http://www.windows.ucar.edu/tour/link=/the_universe/Milkyway.sp.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c10"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Star#/media/File:The_Sun_by_the_Atmospheric_Imaging_Assembly_of_NASA%27s_Solar_Dynamics_Observatory_-_20100819.jpg">Star.jpg</xref> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A large, luminous ball of gas generating energy + internally by nuclear fusion.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">While the behavior of stars forming by accretion + is reasonably well understood,the consequences of merging have not + been fully investermSecated.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una enorme y densa bola de gas que genera fusión + nuclear, liberando así una gran cantidad de energía</descrip> + <admin type="source">spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</admin> + </descripGrp> + <termSec> + <term>estrella</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las estrellas son enormes aglomeraciones de gas, + principalmente Hidrogeno, cuya temperatura es tan alta debido a la + fusión de este elemento, que irradian luz a lo largo de todo el + espectro electromagnético. Poseen diferentes temperaturas que varían + desde los 2000 grados Celsius hasta los 50000.</descrip> + <admin type="source">http://www.astrosurf.com/astronosur/estrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c11"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Ultraviolet#/media/File:UV_LED_Fluoresence.jpg">UV_Radiation.jpg</xref> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The region of the electromagnetic spectrum + spanning the wavelength range from the Lymann limit at 91.2 nm to 350 + nm.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>UV radiation</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">UV radiation from stars and shocks likely + provide the minimum level of ionization required to couple these + fields strongly to the entangled medium.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">Ultraviolet (UV) radiation is part of the + electromagnetic spectrum emitted by the sun. </descrip> + <admin type="source">http://www.who.int/uv/en/</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">La radiación electromagnética cuya longitud de + onda está comprendida aproximadamente entre los 400 nm y los 15 + nm.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Radiaci%C3%B3n_UV</admin> + </descripGrp> + <termSec> + <term>radiación UV</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">Los usuarios de camas solares se someten a dosis + considerables de radiaciones UV artificiales para conseguir un + bronceado complementario al obtenido al tomar el sol.</descrip> + <admin type="source">http://copublications.greenfacts.org/es/camas-solares/</admin> + </descripGrp> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">La radiación ultravioleta se encuentra entre la + luz visible y los rayos X del espectro electromagnético.</descrip> + <admin type="source">http://www.windows.ucar.edu/tour/link=/physical_science/magnetism/em_ultraviolet.sp.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c12"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Magnetic_field#/media/File:VFPt_magnets_BHM.svg">Magnetic_Field.jpg</xref> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A region subject to the influence of magnetism + that is manifested by the mechanical forces that it exerts upon + electricity moving across it and upon the poles of magnets placed in + it.</descrip> + <admin type="source">Merriam-Webster2002</admin> + </descripGrp> + <termSec> + <term>magnetic field</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Detailed consideration of the merger process + will require numerical modeling in which the hydrodynamics, effects + of gravity,magnetic fields, and radiation are considered + carefully.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un campo de fuerza creado como consecuencia del + movimiento de cargas eléctricas, del flujo de la electricidad.</descrip> + <admin type="source">http://www.greenfacts.org/es/glosario/abc/campo-magnetico.htm</admin> + </descripGrp> + <termSec> + <term>campo magnético</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El campo magnético es producido por la corriente + eléctrica que circula por un conductor.</descrip> + <admin type="source">http://teleformacion.edu.aytolacoruna.es/FISICA/document/teoria/A_Franco/elecmagnet/magnetico/cMagnetico.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c13"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Blue_straggler#/media/File:Ngc6397_hst_blue_straggler.jpg">Blue_Straggler.jpg</xref> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A blue main-sequence star, usually found in a + globular or open cluster that appears to be slower in its evolution than + other stars of similar mass and luminosity in the same + cluster.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>blue straggler</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Numerical models of stellar collisions leading + to the formation of blue stragglers in globular clusters (Lombardi + et al. 2002, 2003; Fregeau et al. 2004) indicate that merger + products have radii up to 30 times larger than that of an equivalent + main-sequence star.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Estrellas que aparentan una edad menor que la del + sistema estelar al que pertenecen, si se supone que se formaron junto + con él.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Estrella_rezagada_azul</admin> + </descripGrp> + <termSec> + <term>estrella rezagada azul</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Las últimas observaciones de las “rezagadas + azules”, estrellas atípicas que aparentan ser más jóvenes que el + sistema estelar al que pertenecen, han proporcionado dos modelos + diferentes sobre su origen.</descrip> + <admin type="source">http://mundoastronomia.portalmundos.com/nuevas-pistas-sobre-el-origen-de-las-estrellas-rezagadas-azules/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c14"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The sudden collapse of a massive star when the + internal pressure pushing outwards falls so that it cannot balance the + weight of material pressing inward.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>gravitational collapse</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Stars form from the gravitational collapse of + turbulent molecular cloud cores (Elmegreen & Scalo 2004; Mac Low + & Klessen 2004).</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado final de la evolución de una estrella + de gran masa en el que la materia se comprime bajo la acción de su + propia atracción gravitatoria, con desprendimiento de grandes cantidades + de energía.</descrip> + <admin type="source">http://www.conocimientosweb.net/portal/term6172.html</admin> + </descripGrp> + <termSec> + <term>colapso gravitacional</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Esto sucede si la masa de un pedazo de la nube + excede cierto valor crítico, de modo tal que la fuerza de gravedad + vence definitivamente y el pedazo empieza a contraerse, aumentando + su densidad. Este proceso se llama colapso gravitacional. </descrip> + <admin type="source">http://bibliotecadigital.ilce.edu.mx/sites/ciencia/volumen1/ciencia2/06/html/sec_15.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c15"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Binary_star#/media/File:Algol_AB_movie_imaged_with_the_CHARA_interferometer_-_labeled.gif">Binary_Star.jpg</xref> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A pair of stars in orbit around each other, held + together by the graviational attraction between them.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>binary star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">These authors considered collision partners + having similar masses and concluded that such interactions can at + most account for a small fraction of the observed binary star + population in young clusters.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un sistema estelar compuesto de dos estrellas que + orbitan mutuamente alrededor de un centro de masas común.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Estrella_binaria</admin> + </descripGrp> + <termSec> + <term>estrella binaria</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">La explosión de una estrella binaria dentro de + una nebulosa planetaria ha sido capturado por un equipo dirigido por + investermSecadores del University College of London UCL - es un + acontecimiento que no ha sido presenciado hace más de 100 + años.</descrip> + <admin type="source">http://www.astroelche.es/blog/index.php?blog=2&title=astronomos-capturam-la-explosion-de-una-&more=1&c=1&tb=1&pb=1</admin> + </descripGrp> + </termSec> + <termSec> + <term>estrella doble</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Una estrella doble es una pareja de estrellas + que se mantienen unidas por la fuerza de la gravitación y giran en + torno a su centro común.</descrip> + <admin type="source">http://www.astromia.com/universo/dobles.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c16"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Initial_mass_function#/media/File:LH_95.jpg" + >Initial_Mass_Function.JPG</xref> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A mathematical description of the relative + frequncy with which stars of various masses are formed.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>initial mass function</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The extremely rare merger of two stars close to + the upper-mass end of the initial mass function may be a possible + pathway to hypernova-generated gamma-ray bursts.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-17</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">La expresión numérica que determina el número de + estrellas con masa en un rango determinado.</descrip> + <admin type="source">Basado en http://laeff.cab.inta-csic.es/modules.php?op=modload&name=phpWiki&file=index&pagename=Research-Estrellas-IMF</admin> + </descripGrp> + <termSec> + <term>función inicial de masa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Estado evolutivo y función inicial de masa de + cúmulos jóvenes en la gran nube de Magallanes (estudio en el + ultravioleta).</descrip> + <admin type="source">http://dialnet.unirioja.es/servlet/tesis?codigo=11651</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c17"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Bally2005</term> + + + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c18"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Cambridge2007</term> + + + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c19"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Merriam-Webster2002</term> + + + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c20"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <termSec> + <term>Oxford2007</term> + + + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c21"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Supernova#/media/File:SN1994D.jpg">Supernova.jpg</xref> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A catastrophic stellar explosion in which so much + energy is released that the supernova alone can outshine an entire + galaxy of billions of stars.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <termSec> + <term>supernova</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The supermassive object may be eventually + disrupted by an unusually violent supernova explosion (a hypernova) + soon after formation.</descrip> + <admin type="source">Bally2005</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-20</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Student</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella que estalla y lanza a todo su + alrededor la mayor parte de su masa a altísimas velocidades.</descrip> + <admin type="source">http://www.astromia.com/glosario/supernova.htm</admin> + </descripGrp> + <termSec> + <term>supernova</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Un equipo de científicos británicos propone esta + semana en la revista Nature que la tenue supernova SN2008ha, + descubierta por una adolescente estadounidense en noviembre de 2008, + podría ser la explosión de una estrella masiva, en lugar de proceder + de una enana blanca como se planteaba hasta ahora.</descrip> + <admin type="source">http://www.plataformasinc.es/index.php/esl/Noticias/Una-supernova-observada-por-astronomos-aficionados-abre-el-debate-entre-los-profesionales</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c22"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>Moore2003</term> + + + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c23"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Red_giant#/media/File:Mira_1997.jpg">Red_Giant.jpg</xref> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cool, large and highly luminous star that has + left the main sequence and is powered by heavier elements than + hydrogen.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>red giant</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The core temperature becomes so high that helium + start to 'burn', producing carbon; around this active core there is + a shell where hydrogen is still producing energy. The star becomes + unstable, and the outer layers swell out, cooling as they do so. The + star becomes a red giant.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella de masa baja o intermedia (menos de + 8-9 masas solares) que, tras haber consumido el hidrógeno en su núcleo + durante la etapa de secuencia principal, convirtiéndolo en helio por + fusión nuclear, comienza a quemar hidrógeno en una cáscara alrededor del + núcleo de helio inerte.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Gigante_roja</admin> + </descripGrp> + <termSec> + <term>gigante roja</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">La gigante roja S Orionis (S Ori) es una + estrella variable del tipo Mira. Su masa es similar a la del Sol, + con la diferencia de que está mucho más cerca de convertirse en una + enana blanca, el mismo final que le espera a nuestro Sol dentro de 5 + mil millones de años.</descrip> + <admin type="source">http://www.solociencia.com/astronomia/07071709.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c24"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Red_dwarf#/media/File:New_shot_of_Proxima_Centauri,_our_nearest_neighbour.jpg">Red_Dwarf.jpg</xref> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cool, faint, low-mass star lying at the lower + end of the main sequence of spectral type K or M.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>red dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The dim red dward Proxima, more than a degree + away from Alpha, is slightly closer to us.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella pequeña y relativamente fría de la + secuencia principal, ya sea de tipo espectral K tardío o M.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Enana_roja</admin> + </descripGrp> + <termSec> + <term>enana roja</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El planeta que se ha descubierto girando + alrededor de esta enana roja tiene una masa equivalente a la de + Neptuno, es decir, es sólo 17 veces mayor que la Tierra y mucho + menor que Saturno.</descrip> + <admin type="source">http://axxon.com.ar/not/157/c-1570034.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c25"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Stellar_classification#/media/File:Zeta_Puppis.png">Spectral_Type.jpg</xref> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A means of classifying stars according to the + details of their spectrum, depending largely on their surface + temperature.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>spectral type</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">In this version of a typical HR diagram, the + stars are plotted according to their spectral types and suface + temperatures (horzontal axis, x) and their luminositites in therms + of the Sun (vertical axis, y).</descrip> + <admin type="source">Moore2003, 171</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El espectro de una estrella clasificado por una + letra (O, B, A, F, G, K, M, R, N, S) seguida de un digito que describe + el color de la estrella y su temperatura.</descrip> + <admin type="source">Basado en http://www.espacioprofundo.com.ar/diccionario/Glosario_de_Astronomia/vertermino/Tipo_espectral.html</admin> + </descripGrp> + <termSec> + <term>tipo espectral</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En el gráfico superior se muestra la intensidad + de las líneas espectrales según la temperatura de la estrella (tipo + espectral)</descrip> + <admin type="source">http://www.astrosurf.com/astronosur/estrellas.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c26"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/White_dwarf#/media/File:Sirius_A_and_B_Hubble_photo.editted.PNG">White_Dwarf.jpg</xref> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A small dense star that is has run out of fuel + for nuclear fusion, collapsing under its own gravity and blowing off its + outer layers to form a planetary nebula in the process.</descrip> + <admin type="source">Based on Oxford2007 and Cambridge2007</admin> + </descripGrp> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">To the upper right lie giants and supergiants of + tremendous luminosity, while to the lower left there are the white + dwarfs, which are in a differnt category and were not known when HR + Diagrams were introduced.</descrip> + <admin type="source">Moore2003, 170</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un remanente estelar que se genera cuando una + estrella de masa menor a 9-10 masas solares ha agotado su combustible + nuclear.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Enana_blanca</admin> + </descripGrp> + <termSec> + <term>enana blanca</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Cuando el material fusionable se agota la + estrella pierde la presión interna producida por la fusión nuclear y + puede colapsar inmediatamente terminando en una enana + blanca.</descrip> + <admin type="source">http://astroverada.com/_/Main/T_evolucion.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c27"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Planetary_nebula#/media/File:NGC6543.jpg">Planetary_Nebula.jpg</xref> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A bright cloud of glowing gas and dust + surrounding a highly evolved star.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The star's outer layers are thrown off, and for + a cosmically brief period - no more than about 100,000 years - we + have the phenomenon of what is termed a planetary nebula.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una nebulosa de emisión consistente en una + envoltura brillante en expansión de plasma y gas ionizado, expulsada + durante la fase de rama asintótica gigante que atraviesan las estrellas + gigantes rojas en los últimos momentos de sus vidas.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Nebulosa_planetaria</admin> + </descripGrp> + <termSec> + <term>nebulosa planetaria</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las nebulosas planetarias resultan objetos muy + espectaculares si se observan con un telescopio de media o gran + potencia.</descrip> + <admin type="source">http://www.astromia.com/glosario/nebulosaplanetaria.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c28"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Emission_nebula#/media/File:Ring_Nebula.jpg">Emission_Nebula.jpg</xref> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A luminous cloud of gas and sust in space which + shines with its own light, which can be generated in several + ways.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">In this and other similar emission nebulae, + energetic ultraviolet light from a hot young star strips electrons + from the surrounding hydrogen atoms.</descrip> + <admin type="source">http://apod.nasa.gov/apod/emission_nebulae.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una nube de gas interestelar que brilla por la + excitación del gas, causado por radiación ultravioleta emitida por + estrellas inmersas en la nube o por calentamiento debido a otro + mecanismos. </descrip> + <admin type="source">http://www.diclib.com/Nebulosa%20de%20emisi%C3%B3n/show/en/es_astronomia/726</admin> + </descripGrp> + <termSec> + <term>nebulosa de emisión</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las nebulosas de emisión estan normalmente en + los lugares de formación de estrellas.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c29"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Nebula#/media/File:Eagle_nebula_pillars.jpg">Nebula.jpg</xref> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cloud of interstellar gas and dust.</descrip> + <admin type="source">Cambridge2007</admin> + </descripGrp> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: singular</note> + <descripGrp> + <descrip type="context">According to current theory, a star begins by + condensing out of the tenuous material making up a nebula.</descrip> + <admin type="source">Moore2003, 172</admin> + </descripGrp> + </termSec> + <termSec> + <term>nebulae</term> + + + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: plural</note> + <descripGrp> + <descrip type="context">Other nebulae are within the range of small + telescopes.</descrip> + <admin type="source">Moore2003, 187</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-24</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Regiones del medio interestelar constituidas por + gases (principalmente hidrógeno y helio) y polvo.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Nebulosa</admin> + </descripGrp> + <termSec> + <term>nebulosa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">A unos 1.500 años-luz de distancia, dentro de + nuestro brazo espiral en la Vía Láctea, la Nebulosa de Orión está en + el centro de la región de la Espada de la constelación de Orión el + Cazador, que domina el cielo nocturno a inicios del invierno, en las + latitudes Norte.</descrip> + <admin type="source">http://www.oarval.org/OrionNebsp.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c30"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Dark_nebula#/media/File:All_Quiet_in_the_Nursery%3F.jpg">Dark_Nebula.jpg</xref> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A type of interstellar cloud that is so dense + that it obscures the light from the background emission or reflection + nebula or that it blocks out background stars.</descrip> + <admin type="source">http://en.wikipedia.org/wiki/Dark_nebula</admin> + </descripGrp> + <termSec> + <term>dark nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">There is no difference between a dark nebula and + a bright one, except for the lack of illumination.</descrip> + <admin type="source">Moore2003, 187</admin> + </descripGrp> + </termSec> + <termSec> + <term>absorbtion nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">An absorption nebula is a dense cloud of dust + and gas. From the point of view of an observer on Earth, it absorbs + the light from more distant stars, creating a dark, starless + region.</descrip> + <admin type="source">http://www.glyphweb.com/esky/concepts/absorptionnebula.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Nubes de polvo que simplemente tapan la luz de lo + que haya detras.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + <termSec> + <term>nebulosa oscura</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <descripGrp> + <descrip type="context">Aqui hay un mapa que muestra las regiones de + nebulosas oscuras que estan en un radio de 2000 años luz.</descrip> + <admin type="source">http://www.atlasoftheuniverse.com/espanol/darknebs.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">El caso más opuesto a las nebulosas de emisión + son las nebulosas de absorción (nebulosas oscuras). Estas ni si + quiera están rodeadas de estrellas lo suficientemente potentes ni + cercanas para hacer llegar la luminosidad suficiente para que la + nebulosa pueda reflejarla.</descrip> + <admin type="source">http://www.blogdeastronomia.es/astronomia/formacion-de-estrellas/las-nebulosas</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c31"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Birth</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Reflection_nebula#/media/File:Reflection.nebula.arp.750pix.jpg">Reflection_Nebula.jpeg</xref> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A cloud of interstellar gas and dust that appears + bight because it reflects or scatters starlight.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>reflection nebula</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Just weeks after NASA astronauts repaired the + Hubble Space Telescope in December 1999, the Hubble Heritage Project + snapped this picture of NGC 1999, a reflection nebula in the + constellation Orion. </descrip> + <admin type="source">http://www.nasa.gov/multimedia/imagegallery/image_feature_701.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-28</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Nubes de polvo que simplemente reflejan la luz de + una estrella o estrellas cercanas.</descrip> + <admin type="source">http://www.astrored.net/nebulosaweb/types.html</admin> + </descripGrp> + <termSec> + <term>nebulosa de reflexión</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Como el propio nombre implica, esta nebulosa de + reflexión asociada con la estrella Rigel, se asemeja a una vieja + arpía de un cuento de hadas. </descrip> + <admin type="source">http://www.astrofotos.com.es/2008/11/nebulosa-de-la-cabeza-de-bruja.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c32"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Neutron_star#/media/File:PIA18848-PSRB1509-58-ChandraXRay-WiseIR-20141023.jpg">Neutron_Star.jpg</xref> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">After its Main Sequence period the star becomes + a red supergiant and may explode as a supernova. It may end as a + neutron star or pulsar, although if its mass is even greater it may + poroduce a black hole.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <descripGrp> + <descrip type="definition">Un cuerpo pequeño muy denso que se forma en el + envejecimiento de una estrella pesada y que está formada únicamente por + partículas subatómicas denominadas neutrones.</descrip> + <admin type="source">http://www.astroasa.com.ar/diccionario_astro.htm</admin> + </descripGrp> + <termSec> + <term>estrella de neutrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">El Gran Telescopio Canarias (GTC), instalado en + el Observatorio del Roque de los Muchachos (La Palma), ha obtenido + imágenes de una profundidad "sin precedentes" de una estrella de + neutrones del tipo magnetar, de las que se conocen seis, según ha + informado el Instituto de Astrofísica de Canarias (IAC).</descrip> + <admin type="source">http://www.rtve.es/noticias/20100301/imagen-unica-estrella-neutrones-cazada-canarias/321412.shtml</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c33"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The maximum possible mass of a degenerate star, + above which it will be unable to support itself against the inward pull + of its own gravity. </descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">However, there is a limit, once the mass of the + white dwarf becomes greater than 1.4 time that of the sun )a value + known as the Chandrasekhar limit, after the Indian astronomer who + first worked it out=, the carbon detonates, and in a matter of a few + seconds the white dwarf blows itself to pieces.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El límite de masa más allá del cual la + degeneración de electrones no es capaz de contrarrestar la fuerza de + gravedad en un remanente estelar, produciéndose un colapso que origina + una estrella de neutrones o un agujero negro. </descrip> + <admin type="source">http://es.wikipedia.org/wiki/L%C3%ADmite_de_Chandrasekhar</admin> + </descripGrp> + <termSec> + <term>límite de Chandrasekhar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Descubrió una masa (aproximadamente 1.5 veces la + masa del Sol) en la que una estrella fría no podría soportar su + gravedad. Esto es lo que se conoce como el límite de + Chandrasekhar.</descrip> + <admin type="source">http://html.rincondelvago.com/agujeros-negros_5.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c34"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The state of degeneracy attained when the density + of matter is so high that neutrons cannot be packed any more closely + together.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado de degeneración alcanzado cuando la + densidad de materia es tan alta, que los neutrones no pueden juntarse + más.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>degeneración de neutrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c35"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The radius of the event horizon of a black + hole.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>Schwarzschild radius</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">The critical radius of a non-rotating black hole + is called the Schwarzschild radius, after the German astronomer who + investermSecated the problem mathematically as long ago as 1916: the + boundary around the collapsed star having this radius is termed the + 'event horizon'.</descrip> + <admin type="source">Moore2003</admin> + </descripGrp> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El radio del horizonte de sucesos para un agujero + negro.</descrip> + <admin type="source">http://www.astrocosmo.cl/glosario/glosar-r.htm</admin> + </descripGrp> + <termSec> + <term>radio de Schwarzschild</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Me pareció muy interesante este vídeo del + proyecto Sixty Symbols de la Universidad de Nottingham en el que + explican de forma divulgativa qué es el radio de Schwarzschild. + Básicamente es el radio de un agujero negro.</descrip> + <admin type="source">http://www.microsiervos.com/archivo/ciencia/agujeros-negros-y-el-radio-de-schwarzschild.html</admin> + </descripGrp> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c36"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The surface of a black hole.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>event horizon</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Narayan and Heyl have calculated that if very + heavy objects do not collapse to a point with an event horizon but + instead have a surface, they would eject as many type 1 bursts as + neutron stars.</descrip> + <admin type="source">http://www.newscientist.com/article/dn2527-astronomers-reach-the-event-horizon.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El superficie de un agujero negro.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>horizonte de sucesos</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">En consecuencia, aquí, cuando nos estamos + refiriendo a una «singularidad», estamos pensando en una masa con + volumen nulo rodeada de una frontera gravitacional llamada + «horizonte de sucesos», de la cual nada puede escapar. </descrip> + <admin type="source">http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>horizonte de eventos</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">InvestermSecadores de la Universidad de St. Andrews + en Escocia, afirman haber encontrado una forma de simular un + horizonte de eventos de un agujero negro – no a través de una nueva + técnica de observación cósmica, ni mediante una supercomputadora de + alta potencia … sino en el laboratorio.</descrip> + <admin type="source">http://www.cienciakanija.com/2008/02/14/horizonte-de-eventos-sintetico-de-un-agujero-negro-creado-en-un-laboratorio-del-reino-unido/</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c37"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Proton%E2%80%93proton_chain_reaction#/media/File:Fusion_in_the_Sun.svg">PP_Chain.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>proton-proton chain reaction</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">The proton–proton chain reaction is one of + several fusion reactions by which stars convert hydrogen to helium, + the primary alternative being the CNO cycle. The proton–proton chain + dominates in stars the size of the Sun or smaller.</descrip> + <admin type="source">http://www.absoluteastronomy.com/topics/Proton-proton_chain_reaction</admin> + </descripGrp> + </termSec> + <termSec> + <term>PP chain</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">The primary reactions in the main branch of the + PP chain are illustrated in the following figure.</descrip> + <admin type="source">http://csep10.phys.utk.edu/astr162/lect/energy/ppchain.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>proton-proton reaction</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The gamma rays produced in the proton-proton + reaction take one to 10 million years to work their way out from the + star's core, being scattered numerous times and losing energy as + they go, until they emerge from the surface as rays of light and + heat. Inside the Sun, about 655 million tons of hydrogen are + converted into 650 million tons of helium every second. In stars + heavier than about 2 solar masses, in which the core temperature is + more than about 18 million K, the dominant process in which energy + is produced by the fusion of hydrogen into helium is a different + reaction chain known as the carbon-nitrogen cycle. </descrip> + <admin type="source">http://www.daviddarling.info/encyclopedia/P/proton-proton_chain.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un conjunto de procesos nucleares mediante los + cuales cuatro núcleos de átomos de hidrógeno se combinan para formar uno + de helio, produciendo gran cantidad de energía.</descrip> + <admin type="source">http://www.avizora.com/publicaciones/astronomia/textos/glosario_astronomia_afines_0006.htm</admin> + </descripGrp> + <termSec> + <term>cadena protón-protón</term> + + + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c38"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/CNO_cycle#/media/File:CNO_cycle.png">CNO_Cycle.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>carbon-nitrogen cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The Helium burning process are important 1) + Carbon-Nitrogen cycle at which a carbon-12 nucleus (12C) capture + proton and is converted into 13C, Nitrogen-4 and nitrogen –15. </descrip> + <admin type="source">http://www.sciencenews.org/view/generic/id/44769/title/Supernova_may_be_in_a_new_class</admin> + </descripGrp> + </termSec> + <termSec> + <term>CNO cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</descrip> + <admin type="source">http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">For stars heavier than the sun, theoretical + models show that the CNO (carbon-nitrogen-oxygen) cycle of nuclear + fusion is the dominant source of energy generation.</descrip> + <admin type="source">http://nobelprize.org/nobel_prizes/physics/articles/fusion/sun_cno.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Dr. von Weizsäcker is best known in science for + what is sometimes called the Bethe-Weizsäcker cycle, proposed by him + and the physicist Hans Bethe in the late 1930s as the nuclear + reactive process by which energy is generated in stars. </descrip> + <admin type="source">http://www.nytimes.com/2007/05/02/world/europe/02weizsacker.html</admin> + </descripGrp> + </termSec> + <termSec> + <term>carbon cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">The main theme of the carbon cycle is the adding + of protons, but after a carbon-12 nucleus fuses with a proton to + form nitrogen-13, one of the protons decays with the emission of a + positron and a neutrino to form carbon -13.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/carbcyc.html</admin> + </descripGrp> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">We argue that it may be possible to exploit + neutrinos from the CN cycle and p-p chain to determine the + primordial solar core abundances of C and N at an interesting level + of precision.</descrip> + <admin type="source">http://iopscience.iop.org/0004-637X/687/1/678</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>ciclo CNO</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <termNote type="termType">shortForm</termNote> + <descripGrp> + <descrip type="context">Existen dos formas fundamentales en las que una + estrella fusiona hidrógeno para producir helio: la cadena + protón-protón y el ciclo CNO.</descrip> + <admin type="source">http://eltamiz.com/2007/09/06/la-vida-privada-de-las-estrellas-las-entranas-de-una-estrella/</admin> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <termNote type="termType">fullForm</termNote> + <descripGrp> + <descrip type="context">No se pretende copiar los complicados ciclos de + reacciones que se dan en el interior de las estrellas, como la + cadena protón-protón o el ciclo del carbono-nitrógeno-oxígeno (esta + última más importante en las estrellas más masivas que el Sol). </descrip> + <admin type="source">http://www.zaragoza.es/ciudad/conocimiento/zivis/aplicaciones.htm</admin> + </descripGrp> + </termSec> + <termSec> + <term>ciclo del carbono</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">El ciclo del carbono comienza y acaba con un + núcleo de carbono 12 que actúa como catalizador en la producción de + un núcleo de helio a partir de núcleos de hidrógeno; también se + producen neutrinos y rayos gamma. </descrip> + <admin type="source">http://www.astromia.com/glosario/ciclocno.htm</admin> + </descripGrp> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + <termNote type="termType">variant</termNote> + <descripGrp> + <descrip type="context">En las estrellas de gran masa, que queman su + hidrógeno mucho más rápidamente, predomina el ciclo del + carbono-nitrógeno (CN).</descrip> + <admin type="source">http://www.aavbae.net/bol17/evolucion.php</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c39"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A state of matter attained when atomic particles + are packed together as termSechtly as is physically possible, at densities + of several thousand tonnes per cubic metre.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Although Eddington raised doubts at the meeting + about the concept of relativistic degeneracy, astronomy has since + found that all white dwarfs for which masses have been measured fall + neatly below the Chandrasekhar limit without exception. Today there + are no doubts about his work on degeneracy. </descrip> + <admin type="source">http://www.tamil.net/people/andrew/subra.htm</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Estado de la materia producido cuando las + partículas atómicas tienen el mayor empaquetamiento físicamente posible, + con densidades de varios miles de toneladas por centímetro cúbico. </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + <termSec> + <term>degeneración</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Estas estrellas son aún más densas que las + enanas blancas, y más pequeñas. Se mantienen por un proceso de + "degeneración de neutrones" o "repulsión de neutrones".</descrip> + <admin type="source">http://www.austrinus.com/index.php?option=com_content&view=article&id=157&Itemid=112</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c40"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <langSec xml:lang="zu"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <termSec> + <term>Oxford2003</term> + + + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c41"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The state of degeneracy attained when the density + of matter is so high that electrons cannot be packed any closer + together.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">When it reaches the threshold of energy + necessary to force the combining of electrons and protons to form + neutrons, the electron degeneracy limit has been passed and the + collapse continues until it is stopped by neutron + degeneracy.</descrip> + <admin type="source">http://hyperphysics.phy-astr.gsu.edu/HBASE/Astro/pulsar.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El estado de degeneración alcanzado cuando la + densidad de materia es tan grande, que los electrones no pueden + empaquetarse más.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>degeneración de electrones</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Es la principal responsable de la resistencia al + colapso gravitacional de las enanas blancas (degeneración de + electrones) y de las estrellas de neutrones (degeneración de + neutrones). </descrip> + <admin type="source">http://www.emiliosilveravazquez.com/glosario.php?letra=d</admin> + </descripGrp> + </termSec> + <termSec> + <term>degeneración electrónica</term> + + + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <descripGrp> + <descrip type="context">Las fuerzas gravitatorias actuantes en un cuerpo + celeste masivo pueden comprimir su materia hasta un estado de + degeneración electrónica y no más, ya que el principio de exclusión + impide a dos electrones ocupar el mismo nivel de energía. </descrip> + <admin type="source">http://www.portalplanetasedna.com.ar/estrella2.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c42"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-05-01</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Event_horizon#/media/File:Spacetime_lattice_analogy.svg">Event_Horizon.jpg</xref> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A mathematical point at which certain physical + quantities reach infinite values.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>singularity</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">A singularity means a point where some property + is infinite. For example, at the center of a black hole, according + to classical theory, the density is infinite (because a finite mass + is compressed to a zero volume). Hence it is a singularity. </descrip> + <admin type="source">http://curious.astro.cornell.edu/question.php?number=55</admin> + </descripGrp> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Un punto matemático en el que ciertas cantidades + físicas alcanzan valores infinitos.</descrip> + <admin type="source">Oxford2003</admin> + </descripGrp> + <termSec> + <term>singularidad</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Las singularidades ocurren en el Big Bang, en + los agujeros negros y en el Big Crunch (que podría ser considerado + como una unión de agujeros negros).</descrip> + <admin type="source">http://www.astrocosmo.cl/h-foton/h-foton-03_08-01.htm</admin> + </descripGrp> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c43"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Solar_mass#/media/File:Rho_Cassiopeiae_Sol_VY_Canis_Majoris.png">Solar_Mass.jpg</xref> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A unit of mass used in stellar and galactic + astronomy, equivalent to the mass of the sun, 1.989 x 10^30 + kg.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>solar mass</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">This page now explores the fate of stars of 8 + solar masses or less.</descrip> + <admin type="source">http://outreach.atnf.csiro.au/education/senior/astrophysics/stellarevolution_deathlow.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una unidad de medida utilizada en astronomía y + astrofísica para medir comparativamente la masa de las estrellas y otros + objetos astronómicos muy masivos como galaxias.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Masa_solar</admin> + </descripGrp> + <termSec> + <term>masa solar</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Para una nube con la masa de nuestro Sol, el + colapso dura unos 10 millones de años, mientras que si su masa fuese + mucho más pequeña, por ejemplo un décimo de la masa solar, este + proceso podría durar hasta 800 millones de años.</descrip> + <admin type="source">http://www.tayabeixo.org/sist_solar/hipotesis/formacion_sistsolar.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c44"> + <descrip type="subjectField">General</descrip> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Triple-alpha_process#/media/File:Triple-Alpha_Process.svg" + >Triple-Alpha_Process.jpg</xref> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">The chain of nuclear reactions by which carbon is + synthesized in the interiors of stars through the fusion of three helium + nuclei(alpha particles).</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>triple-alpha process</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">This small concentration of Be-8 can begin to + undergo reactions with other He-4 nuclei to produce an excited state + of the mass-12 isotope of Carbon. This excited state is unstable, + but a few of these excited Carbon nuclei emit a gamma-ray quickly + enough to become stable before they disintegrate. This extremely + improbable sequence is called the triple-alpha process because the + net effect is to combine 3 alpha particles (that is, 3 He-4 nuclei) + to form a C-12 nucleus. </descrip> + <admin type="source">http://csep10.phys.utk.edu/astr162/lect/energy/triplealph.html</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">El proceso por el cual tres núcleos de helio + (partículas alfa) se transforman en un núcleo de carbono.</descrip> + <admin type="source">http://es.wikipedia.org/wiki/Proceso_triple-alfa</admin> + </descripGrp> + <termSec> + <term>proceso triple-alfa</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">También debe tenerse en cuenta una tercera + reacción de gran importancia, denominada proceso triple + alfa.</descrip> + <admin type="source">http://feinstein.com.ar/Composicion.html</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + + + <conceptEntry id="c45"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descrip type="subjectField">General</descrip> + <xref type="xGraphic" target="https://en.wikipedia.org/wiki/Black_dwarf#/media/File:Black_dwarf.jpg">Black_Dwarf.jpg</xref> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">A degenerate star that has cooled until it is no + longer visible.</descrip> + <admin type="source">Oxford2007</admin> + </descripGrp> + <termSec> + <term>black dwarf</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">Banprupt though it is, a white swarf still has a + high surface temperature when it is first formed; up to 100,000 + degrees C in some cases and it continues to radiate. Gradually it + fades, and must end up as a cold, dead black dwarf; but at the + moment no white dwarf with a surface temperature of below 3,000 + degrees C has been found, and it may be that the universe is not yet + old enough for any black dwarfs to have been formed.</descrip> + <admin type="source">Moore2003, 173</admin> + </descripGrp> + </termSec> + </langSec> + <langSec xml:lang="es"> + <transacGrp> + <transac type="transactionType">creation</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <transacGrp> + <transac type="transactionType">modification</transac> + <date>2010-04-29</date> + <transacNote type="responsibility" target="pe324as3-9615-4d41-a9c8-30c36bffe0e6">Tommy</transacNote> + </transacGrp> + <descripGrp> + <descrip type="definition">Una estrella creada cuando una enana blanca se + enfría lo suficiente como para dejar de emitir calor o luz en cantidad + significativa.</descrip> + <admin type="source">http://spaceplace.nasa.gov/sp/kids/spitzer/signs/sign_glossary.shtml</admin> + </descripGrp> + <termSec> + <term>enana negra</term> + + + <termNote type="partOfSpeech">noun</termNote> + <descripGrp> + <descrip type="context">No se conoce, todavía, la cantidad de Enanas + Negras que pueblan en realidad nuestro Universo. El tiempo estimado + para que una Enana Blanca se enfríe lo suficiente para volverse + Negra, se estima entre diez y cien mil millones de años, y nuestro + Universo no es aún lo bastante viejo, nada más que para que existan + algunas enanas blancas que se han enfriado lo suficiente para + alcanzar la etapa de enanas negras.</descrip> + <admin type="source">http://celestia.albacete.org/celestia/celestia/stars/enana12.htm</admin> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> + +</tbx> diff --git a/spec/fixtures/TBX_test_files/core_structure_bad.tbx b/spec/fixtures/TBX_test_files/core_structure_bad.tbx new file mode 100644 index 0000000..c20b1fd --- /dev/null +++ b/spec/fixtures/TBX_test_files/core_structure_bad.tbx @@ -0,0 +1,780 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<!-- + Expected errors: + - <tbxHeader> descendants' text must be wrapped in <p> + - <admin> may not be direct child of <text> + - <term> must come first in <termSec> + - <admin> must have some type attribute + - only one <term> per <termSec> + - only one <descrip> per <descripGrp> +--> +<tbx type="TBX-Core" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + TBX file, created via MultiTerm Export + </sourceDesc> + </fileDesc> + </tbxHeader> + <text> + <admin type="whateverForCore">Wrong place.</admin> + <body> + <conceptEntry id="c1"> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <termSec> + <admin>No type/wrong order</admin> + <term>Wrong order</term> + </termSec> + <termSec> + <term>galactic cluster</term> + <term>Second term</term> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo abierto</term> + <descripGrp> + <descrip type="whateverType">First descrip in one group.</descrip> + <descrip type="whateverType">Second descrip in one group.</descrip> + </descripGrp> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c2"> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <termSec> + <term>circumstellar accretion disk</term> + </termSec> + <termSec> + <term>accretion disc</term> + </termSec> + <termSec> + <term>circumstellar disk</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>disco de acreción</term> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c3"> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <termSec> + <term>black hole</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>agujero negro</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c4"> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <termSec> + <term>gamma-ray burst</term> + </termSec> + <termSec> + <term>GRB</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>explosión de rayos gamma</term> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c5"> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <termSec> + <term>globular cluster</term> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo globular</term> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c6"> + <langSec xml:lang="en"> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <termSec> + <term>main-sequence</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>de secuencia principal</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c7"> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <termSec> + <term>protostar</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <termSec> + <term>protoestrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c8"> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <termSec> + <term>star cluster</term> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo estelar</term> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c9"> + <langSec xml:lang="en"> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <termSec> + <term>Galaxy</term> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + </termSec> + <termSec> + <term>Milky Way</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <termSec> + <term>Galaxia</term> + </termSec> + <termSec> + <term>Vía Láctea</term> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c10"> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c11"> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>UV radiation</term> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radiación UV</term> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c12"> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>magnetic field</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>campo magnético</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c13"> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>blue straggler</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella rezagada azul</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c14"> + <langSec xml:lang="en"> + <termSec> + <term>gravitational collapse</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>colapso gravitacional</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c15"> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>binary star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella binaria</term> + </termSec> + <termSec> + <term>estrella doble</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c16"> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <termSec> + <term>initial mass function</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>función inicial de masa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c17"> + <langSec xml:lang="zu"> + <termSec> + <term>Bally2005</term> + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c18"> + <langSec xml:lang="zu"> + <termSec> + <term>Cambridge2007</term> + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c19"> + <langSec xml:lang="zu"> + <termSec> + <term>Merriam-Webster2002</term> + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c20"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2007</term> + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c21"> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c22"> + <langSec xml:lang="zu"> + <termSec> + <term>Moore2003</term> + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c23"> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red giant</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>gigante roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c24"> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c25"> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>spectral type</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>tipo espectral</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c26"> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana blanca</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c27"> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa planetaria</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c28"> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de emisión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c29"> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + <note>Grammatical Number: singular</note> + </termSec> + <termSec> + <term>nebulae</term> + <note>Grammatical Number: plural</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c30"> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <termSec> + <term>dark nebula</term> + </termSec> + <termSec> + <term>absorbtion nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa oscura</term> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c31"> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <termSec> + <term>reflection nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de reflexión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c32"> + <langSec xml:lang="en"> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <termSec> + <term>estrella de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c33"> + <langSec xml:lang="en"> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>límite de Chandrasekhar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c34"> + <langSec xml:lang="en"> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c35"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>Schwarzschild radius</term> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radio de Schwarzschild</term> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c36"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>event horizon</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>horizonte de sucesos</term> + </termSec> + <termSec> + <term>horizonte de eventos</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c37"> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>proton-proton chain reaction</term> + </termSec> + <termSec> + <term>PP chain</term> + </termSec> + <termSec> + <term>proton-proton reaction</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cadena protón-protón</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c38"> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>carbon-nitrogen cycle</term> + </termSec> + <termSec> + <term>CNO cycle</term> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + </termSec> + <termSec> + <term>carbon cycle</term> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>ciclo CNO</term> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + </termSec> + <termSec> + <term>ciclo del carbono</term> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c39"> + <langSec xml:lang="en"> + <termSec> + <term>degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c40"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2003</term> + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c41"> + <langSec xml:lang="en"> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de electrones</term> + </termSec> + <termSec> + <term>degeneración electrónica</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c42"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>singularity</term> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>singularidad</term> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c43"> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <termSec> + <term>solar mass</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>masa solar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c44"> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + <termSec> + <term>triple-alpha process</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>proceso triple-alfa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c45"> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>black dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana negra</term> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> +</tbx> diff --git a/spec/fixtures/TBX_test_files/core_structure_good.tbx b/spec/fixtures/TBX_test_files/core_structure_good.tbx new file mode 100644 index 0000000..0598b3d --- /dev/null +++ b/spec/fixtures/TBX_test_files/core_structure_good.tbx @@ -0,0 +1,764 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<tbx type="TBX-Core" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + <text> + <body> + <conceptEntry id="c1"> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <termSec> + <term>open cluster</term> + </termSec> + <termSec> + <term>galactic cluster</term> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo abierto</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c2"> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <termSec> + <term>circumstellar accretion disk</term> + </termSec> + <termSec> + <term>accretion disc</term> + </termSec> + <termSec> + <term>circumstellar disk</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>disco de acreción</term> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c3"> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <termSec> + <term>black hole</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>agujero negro</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c4"> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <termSec> + <term>gamma-ray burst</term> + </termSec> + <termSec> + <term>GRB</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>explosión de rayos gamma</term> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c5"> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <termSec> + <term>globular cluster</term> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo globular</term> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c6"> + <langSec xml:lang="en"> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <termSec> + <term>main-sequence</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>de secuencia principal</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c7"> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <termSec> + <term>protostar</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <termSec> + <term>protoestrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c8"> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <termSec> + <term>star cluster</term> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo estelar</term> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c9"> + <langSec xml:lang="en"> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <termSec> + <term>Galaxy</term> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + </termSec> + <termSec> + <term>Milky Way</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <termSec> + <term>Galaxia</term> + </termSec> + <termSec> + <term>Vía Láctea</term> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c10"> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c11"> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>UV radiation</term> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radiación UV</term> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c12"> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>magnetic field</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>campo magnético</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c13"> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>blue straggler</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella rezagada azul</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c14"> + <langSec xml:lang="en"> + <termSec> + <term>gravitational collapse</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>colapso gravitacional</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c15"> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>binary star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella binaria</term> + </termSec> + <termSec> + <term>estrella doble</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c16"> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <termSec> + <term>initial mass function</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>función inicial de masa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c17"> + <langSec xml:lang="zu"> + <termSec> + <term>Bally2005</term> + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c18"> + <langSec xml:lang="zu"> + <termSec> + <term>Cambridge2007</term> + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c19"> + <langSec xml:lang="zu"> + <termSec> + <term>Merriam-Webster2002</term> + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c20"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2007</term> + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c21"> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c22"> + <langSec xml:lang="zu"> + <termSec> + <term>Moore2003</term> + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c23"> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red giant</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>gigante roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c24"> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c25"> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>spectral type</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>tipo espectral</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c26"> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana blanca</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c27"> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa planetaria</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c28"> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de emisión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c29"> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + <note>Grammatical Number: singular</note> + </termSec> + <termSec> + <term>nebulae</term> + <note>Grammatical Number: plural</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c30"> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <termSec> + <term>dark nebula</term> + </termSec> + <termSec> + <term>absorbtion nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa oscura</term> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c31"> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <termSec> + <term>reflection nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de reflexión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c32"> + <langSec xml:lang="en"> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <termSec> + <term>estrella de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c33"> + <langSec xml:lang="en"> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>límite de Chandrasekhar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c34"> + <langSec xml:lang="en"> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c35"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>Schwarzschild radius</term> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radio de Schwarzschild</term> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c36"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>event horizon</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>horizonte de sucesos</term> + </termSec> + <termSec> + <term>horizonte de eventos</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c37"> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>proton-proton chain reaction</term> + </termSec> + <termSec> + <term>PP chain</term> + </termSec> + <termSec> + <term>proton-proton reaction</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cadena protón-protón</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c38"> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>carbon-nitrogen cycle</term> + </termSec> + <termSec> + <term>CNO cycle</term> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + </termSec> + <termSec> + <term>carbon cycle</term> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>ciclo CNO</term> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + </termSec> + <termSec> + <term>ciclo del carbono</term> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c39"> + <langSec xml:lang="en"> + <termSec> + <term>degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c40"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2003</term> + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c41"> + <langSec xml:lang="en"> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de electrones</term> + </termSec> + <termSec> + <term>degeneración electrónica</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c42"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>singularity</term> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>singularidad</term> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c43"> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <termSec> + <term>solar mass</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>masa solar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c44"> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + <termSec> + <term>triple-alpha process</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>proceso triple-alfa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c45"> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>black dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana negra</term> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> +</tbx> diff --git a/spec/fixtures/TBX_test_files/min_bad.tbx b/spec/fixtures/TBX_test_files/min_bad.tbx new file mode 100644 index 0000000..1208cbc --- /dev/null +++ b/spec/fixtures/TBX_test_files/min_bad.tbx @@ -0,0 +1,946 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<?xml-model href="../../schematrons/min_schema.sch" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?> +<!-- + Expected errors: + - <admin> "source" not allowed + - "usageStatus" takes wrong value + - <xref> not allowed anywere +--> +<tbx type="TBX-Min" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + <text> + <body> + <conceptEntry id="c1"> + <admin type="source">A DCA datcat from TBX-Basic, not TBX-Min</admin> + + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <termSec> + <term>open cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>galactic cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + <xref type="error" target="https://example.com">Xref is not in TBX-Min</xref> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo abierto</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c2"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <termSec> + <term>circumstellar accretion disk</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>accretion disc</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>circumstellar disk</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>disco de acreción</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c3"> + <descrip type="subjectField">Stellar Death</descrip> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <termSec> + <term>black hole</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>agujero negro</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c4"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <termSec> + <term>gamma-ray burst</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>GRB</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>explosión de rayos gamma</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c5"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <termSec> + <term>globular cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo globular</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c6"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <termSec> + <term>main-sequence</term> + <termNote type="partOfSpeech">adjective</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>de secuencia principal</term> + <termNote type="partOfSpeech">adjective</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c7"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <termSec> + <term>protostar</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <termSec> + <term>protoestrella</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c8"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <termSec> + <term>star cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo estelar</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c9"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <termSec> + <term>Galaxy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>Milky Way</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <termSec> + <term>Galaxia</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>Vía Láctea</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c10"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>star</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c11"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>UV radiation</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radiación UV</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c12"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>magnetic field</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>campo magnético</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c13"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>blue straggler</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella rezagada azul</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c14"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <termSec> + <term>gravitational collapse</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>colapso gravitacional</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c15"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>binary star</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella binaria</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>estrella doble</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c16"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <termSec> + <term>initial mass function</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>función inicial de masa</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c17"> + <langSec xml:lang="zu"> + <termSec> + <term>Bally2005</term> + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c18"> + <langSec xml:lang="zu"> + <termSec> + <term>Cambridge2007</term> + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c19"> + <langSec xml:lang="zu"> + <termSec> + <term>Merriam-Webster2002</term> + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c20"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2007</term> + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c21"> + <descrip type="subjectField">Stellar Death</descrip> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <termSec> + <term>supernova</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>supernova</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c22"> + <langSec xml:lang="zu"> + <termSec> + <term>Moore2003</term> + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c23"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red giant</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>gigante roja</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c24"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red dwarf</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana roja</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c25"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>spectral type</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>tipo espectral</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c26"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana blanca</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c27"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa planetaria</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c28"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de emisión</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c29"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: singular</note> + </termSec> + <termSec> + <term>nebulae</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: plural</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c30"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <termSec> + <term>dark nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>absorbtion nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa oscura</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c31"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <termSec> + <term>reflection nebula</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de reflexión</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c32"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <termSec> + <term>estrella de neutrones</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c33"> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>límite de Chandrasekhar</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c34"> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de neutrones</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c35"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>Schwarzschild radius</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radio de Schwarzschild</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c36"> + <descrip type="subjectField">Stellar Death</descrip> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>event horizon</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>horizonte de sucesos</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>horizonte de eventos</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c37"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>proton-proton chain reaction</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>PP chain</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>proton-proton reaction</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cadena protón-protón</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c38"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>carbon-nitrogen cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>CNO cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>carbon cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>ciclo CNO</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">not an allowed value</termNote> + </termSec> + <termSec> + <term>ciclo del carbono</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c39"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <termSec> + <term>degeneracy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c40"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2003</term> + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c41"> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de electrones</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>degeneración electrónica</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c42"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>singularity</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>singularidad</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c43"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <termSec> + <term>solar mass</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>masa solar</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c44"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + <termSec> + <term>triple-alpha process</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>proceso triple-alfa</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c45"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>black dwarf</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana negra</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + </body> + + </text> +</tbx> diff --git a/spec/fixtures/TBX_test_files/min_good.tbx b/spec/fixtures/TBX_test_files/min_good.tbx new file mode 100644 index 0000000..2eb8518 --- /dev/null +++ b/spec/fixtures/TBX_test_files/min_good.tbx @@ -0,0 +1,937 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<?xml-model href="../../schematrons/min_schema.sch" type="application/xml" schematypens="http://purl.oclc.org/dsdl/schematron"?> +<tbx type="TBX-Min" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + <text> + <body> + <conceptEntry id="c1"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <termSec> + <term>open cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>galactic cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo abierto</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c2"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <termSec> + <term>circumstellar accretion disk</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>accretion disc</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>circumstellar disk</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>disco de acreción</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c3"> + <descrip type="subjectField">Stellar Death</descrip> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <termSec> + <term>black hole</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>agujero negro</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c4"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <termSec> + <term>gamma-ray burst</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>GRB</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>explosión de rayos gamma</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c5"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <termSec> + <term>globular cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo globular</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c6"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <termSec> + <term>main-sequence</term> + <termNote type="partOfSpeech">adjective</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>de secuencia principal</term> + <termNote type="partOfSpeech">adjective</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c7"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <termSec> + <term>protostar</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <termSec> + <term>protoestrella</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c8"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <termSec> + <term>star cluster</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo estelar</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c9"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <termSec> + <term>Galaxy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>Milky Way</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <termSec> + <term>Galaxia</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>Vía Láctea</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c10"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>star</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c11"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>UV radiation</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radiación UV</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c12"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>magnetic field</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>campo magnético</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c13"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>blue straggler</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella rezagada azul</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c14"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <termSec> + <term>gravitational collapse</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>colapso gravitacional</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c15"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>binary star</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella binaria</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>estrella doble</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c16"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <termSec> + <term>initial mass function</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>función inicial de masa</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c17"> + <langSec xml:lang="zu"> + <termSec> + <term>Bally2005</term> + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c18"> + <langSec xml:lang="zu"> + <termSec> + <term>Cambridge2007</term> + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c19"> + <langSec xml:lang="zu"> + <termSec> + <term>Merriam-Webster2002</term> + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c20"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2007</term> + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c21"> + <descrip type="subjectField">Stellar Death</descrip> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <termSec> + <term>supernova</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>supernova</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c22"> + <langSec xml:lang="zu"> + <termSec> + <term>Moore2003</term> + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c23"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red giant</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>gigante roja</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c24"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red dwarf</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana roja</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c25"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>spectral type</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>tipo espectral</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c26"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana blanca</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c27"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa planetaria</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c28"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de emisión</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c29"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: singular</note> + </termSec> + <termSec> + <term>nebulae</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Grammatical Number: plural</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c30"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <termSec> + <term>dark nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>absorbtion nebula</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa oscura</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c31"> + <descrip type="subjectField">Stellar Birth</descrip> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <termSec> + <term>reflection nebula</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de reflexión</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c32"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <termSec> + <term>estrella de neutrones</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c33"> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>límite de Chandrasekhar</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c34"> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de neutrones</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c35"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>Schwarzschild radius</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radio de Schwarzschild</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c36"> + <descrip type="subjectField">Stellar Death</descrip> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>event horizon</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>horizonte de sucesos</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + <termSec> + <term>horizonte de eventos</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c37"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>proton-proton chain reaction</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>PP chain</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>proton-proton reaction</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cadena protón-protón</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c38"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>carbon-nitrogen cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>CNO cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>carbon cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>ciclo CNO</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + </termSec> + <termSec> + <term>ciclo del carbono</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">deprecated</termNote> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">preferred</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c39"> + <descrip type="subjectField">General</descrip> + <langSec xml:lang="en"> + <termSec> + <term>degeneracy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c40"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2003</term> + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c41"> + <descrip type="subjectField">Stellar Death</descrip> + <langSec xml:lang="en"> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de electrones</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + <termSec> + <term>degeneración electrónica</term> + <termNote type="partOfSpeech">noun</termNote> + <termNote type="usageStatus">admitted</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c42"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>singularity</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>singularidad</term> + <termNote type="partOfSpeech">noun</termNote> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c43"> + <descrip type="subjectField">General</descrip> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <termSec> + <term>solar mass</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>masa solar</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c44"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + <termSec> + <term>triple-alpha process</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>proceso triple-alfa</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c45"> + <descrip type="subjectField">General</descrip> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>black dwarf</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana negra</term> + <termNote type="partOfSpeech">noun</termNote> + </termSec> + </langSec> + </conceptEntry> + </body> + + </text> +</tbx> diff --git a/spec/fixtures/TBX_test_files/poorly_formed_xml.tbx b/spec/fixtures/TBX_test_files/poorly_formed_xml.tbx new file mode 100644 index 0000000..26f448d --- /dev/null +++ b/spec/fixtures/TBX_test_files/poorly_formed_xml.tbx @@ -0,0 +1,765 @@ +<?xml version="1.0" encoding="utf-8"?> +<?xml-model href="../../coreSchemas/core_schema.rng" type="application/xml" schematypens="http://relaxng.org/ns/structure/1.0"?> +<!-- Expected error: there is an end-tag missing. --> +<tbx type="TBX-Min" style="dca" xml:lang="en" xmlns="urn:iso:std:iso:30042:ed-2" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"> + <tbxHeader> + <fileDesc> + <sourceDesc> + <p>TBX file, created via MultiTerm Export</p> + </sourceDesc> + </fileDesc> + </tbxHeader> + <text> + <body> + <conceptEntry id="c1"> + <note>G-Source: http://www.physics.drexel.edu/observatory/dump.shtml</note> + <langSec xml:lang="en"> + <termSec> + <term>open cluster</term> + </termSec> + <termSec> + <term>galactic cluster</term> + <note>Another name for an open star cluster. They are often termed Galactic + Clusters because they are found mainly in the plane of our galaxy. If + you were to view our galaxy from afar, you would find that all the + open/galactic clusters lie within the spiral arms of the galaxy.</note> + <note>N-Source: + http://www.delscope.demon.co.uk/astronomy/glossary.htm#G</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo abierto</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c2"> + <note>G-Source: + http://www.cfht.hawaii.edu/Instruments/Spectroscopy/Espadons/www.ast.obs-mip.fr/users/donati/press/fuori_eng.html</note> + <langSec xml:lang="en"> + <termSec> + <term>missing closing tag + </termSec> + <termSec> + <term>accretion disc</term> + </termSec> + <termSec> + <term>circumstellar disk</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>disco de acreción</term> + </termSec> + <termSec> + <term>disco de acrecimiento</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c3"> + <note>G-Source: http://wallpaper-s.org/12__Supermassive_Black_Hole.htm</note> + <langSec xml:lang="en"> + <termSec> + <term>black hole</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>agujero negro</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c4"> + <note>G-Source: + http://nakedmaninthetree.wordpress.com/2009/02/22/galaxies-and-the-future/</note> + <langSec xml:lang="en"> + <termSec> + <term>gamma-ray burst</term> + </termSec> + <termSec> + <term>GRB</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>explosión de rayos gamma</term> + </termSec> + <termSec> + <term>brote de rayos gamma</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c5"> + <note>G-Source: http://www.astrographics.com/GalleryPrintsIndex/GP0046.html</note> + <langSec xml:lang="en"> + <termSec> + <term>globular cluster</term> + <note>Related Term: star cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo globular</term> + <note>Related Term: cúmulo estelar</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c6"> + <langSec xml:lang="en"> + <note>G-Source: http://www.skyofplenty.com/?page_id=374</note> + <termSec> + <term>main-sequence</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>de secuencia principal</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c7"> + <note>G-Source: http://www.konkoly.hu/KISAG/Science/star/star_intro.html</note> + <langSec xml:lang="en"> + <termSec> + <term>protostar</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://geocities.ws/acarvajaltt/temas/estrellas_nacimiento_estelar.html</note> + <termSec> + <term>protoestrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c8"> + <note>G-Source: http://apod.nasa.gov/apod/ap060109.html</note> + <langSec xml:lang="en"> + <termSec> + <term>star cluster</term> + <note>Related Term: globular cluster</note> + <note>Related Term: open cluster</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cúmulo estelar</term> + </termSec> + <termSec> + <term>cúmulo de estrellas</term> + <note>Related Term: cúmulo globular</note> + <note>Related Term: cúmulo abierto</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c9"> + <langSec xml:lang="en"> + <note>G-Source: http://www.cfa.harvard.edu/~afrebel/milky-way-2.jpg</note> + <termSec> + <term>Galaxy</term> + </termSec> + <termSec> + <term>Milky Way Galaxy</term> + </termSec> + <termSec> + <term>Milky Way</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: http://oacs-unah.edu.hn/an111/vrt/img/via_lactea.jpg</note> + <termSec> + <term>Galaxia</term> + </termSec> + <termSec> + <term>Vía Láctea</term> + </termSec> + <termSec> + <term>galaxia Vía Láctea</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c10"> + <note>G-Source: + http://lh4.ggpht.com/_EuutPdvjcY0/SQ2jGBKWO7I/AAAAAAAAALM/gjDMVimDQc8/005Est.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c11"> + <note>G-Source: http://drdima.files.wordpress.com/2009/05/sun-rays.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>UV radiation</term> + </termSec> + <termSec> + <term>ultraviolet radiation</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radiación UV</term> + </termSec> + <termSec> + <term>radiación ultravioleta</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c12"> + <note>G-Source: http://www.greatdreams.com/magnet1.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>magnetic field</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>campo magnético</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c13"> + <note>G-Source: http://images.spaceref.com/news/2009/ooBlue_Straggler09.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>blue straggler</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella rezagada azul</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c14"> + <langSec xml:lang="en"> + <termSec> + <term>gravitational collapse</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>colapso gravitacional</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c15"> + <note>G-Source: + http://lh6.ggpht.com/_6hgSmco4R9M/SaqplXGqJfI/AAAAAAAAA1k/B3a43_O9VI8/56_Binary_Stars_thumb3.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>binary star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>estrella binaria</term> + </termSec> + <termSec> + <term>estrella doble</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c16"> + <note>G-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <note>This figure compares the IMFs by ploting mass fraction per dex versus mass, + i.e., normalized so that the integral under each curve is unity. They are + assumed to be valid from 0.1 to 120 solar masses.</note> + <note>N-Source: + http://www.astro.ljmu.ac.uk/~ikb/research/imf-use-in-cosmology.html</note> + <langSec xml:lang="en"> + <termSec> + <term>initial mass function</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>función inicial de masa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c17"> + <langSec xml:lang="zu"> + <termSec> + <term>Bally2005</term> + <note>Author[s]: Bally, John and Hans Zinnecker</note> + <note>Journal Title: The Astronomical Journal</note> + <note>Article Title: The Birth of High-Mass Stars: Accertion and/or + Mergers?</note> + <note>Volume: 129</note> + <note>Publication Place: U.S.A.</note> + <note>Publisher: The American Astronomical Society</note> + <note>Publication Year: May 2005</note> + <note>Page(s): 2281-2293</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c18"> + <langSec xml:lang="zu"> + <termSec> + <term>Cambridge2007</term> + <note>Author[s]: Mitton, Jaqueline</note> + <note>Book Title: Cambridge Illustrated Dictionary of Astronomy</note> + <note>Publication Place: New York</note> + <note>Publisher: Cambridge University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c19"> + <langSec xml:lang="zu"> + <termSec> + <term>Merriam-Webster2002</term> + <note>Book Title: Webster's Third New International Dictionary</note> + <note>Editor[s]: Gove, Philip Babcock</note> + <note>Volume: Third Edition</note> + <note>Publication Place: Springfield, Massachusetts</note> + <note>Publisher: Merriam-Webster INC.</note> + <note>Publication Year: 2002</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c20"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2007</term> + <note>Book Title: Oxford Dictionary of Astronomy</note> + <note>Editor[s]: Ridpath, Ian</note> + <note>Volume: Second Edition</note> + <note>Publication Place: New York</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2007</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c21"> + <note>G-Source: + http://jcconwell.wordpress.com/2009/07/24/top-10-ways-the-universe-could-kill-us/supernova/</note> + <langSec xml:lang="en"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>supernova</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c22"> + <langSec xml:lang="zu"> + <termSec> + <term>Moore2003</term> + <note>Author[s]: Moore, Patrick</note> + <note>Book Title: Philip's Atlas of the Universe</note> + <note>Publication Place: Heron Quays, London</note> + <note>Publisher: Philip's</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c23"> + <note>G-Source: + http://www.lcsd.gov.hk/CE/Museum/Space/EducationResource/Universe/framed_e/lecture/ch15/imgs/red_size.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red giant</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>gigante roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c24"> + <note>G-Source: http://www.wolflodge.org/bluestar/h_red_dwarf_02.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>red dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana roja</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c25"> + <note>G-Source: + http://www.astro.columbia.edu/~archung/labs/spring2002/images/spectral_type2.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>spectral type</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>tipo espectral</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c26"> + <note>G-Source: http://www.stsci.edu/~inr/thisweek1/thisweek/WhiteDwarf.gif</note> + <langSec xml:lang="en"> + <note>This is the end-result of all but the most massive of stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>white dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana blanca</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c27"> + <note>G-Source: + http://www.phys.ncku.edu.tw/~astrolab/mirrors/apod_e/image/0901/ngc2818_hheritage_800.jpg</note> + <langSec xml:lang="en"> + <note>As mass is gradually lost, the core of the star becomes more exposed, + ultimately becoming a white dwarf. Also, planetary nebulae have nothing to + do with planets, and are not true nebulae.</note> + <note>N-Source: Based on Oxford2007 and Moore2003, 186</note> + <termSec> + <term>planetary nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa planetaria</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c28"> + <note>G-Source: http://apod.nasa.gov/apod/image/0612/NGC2174_lrg.jpg</note> + <langSec xml:lang="en"> + <note>Ultraviolet radiation, gas cloud collisions, and synchrotron radiation can + all cause the emission nebula to shine.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>emission nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de emisión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c29"> + <note>G-Source: + http://my-blackberry.net/wallpapers/49/m/NASA_-_The_Horsehead_Nebula%2C_B33%2C_Orion_Nebula.jpg</note> + <langSec xml:lang="en"> + <note>The term was originally applied to any object with a fuzzy telescopic + appearance, but with the advent of larger instruments many 'nebulae' were + found to consist of faint stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>nebula</term> + <note>Grammatical Number: singular</note> + </termSec> + <termSec> + <term>nebulae</term> + <note>Grammatical Number: plural</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c30"> + <note>G-Source: http://www.mallorcaweb.net/masm/obstel/caballo.GIF</note> + <langSec xml:lang="en"> + <termSec> + <term>dark nebula</term> + </termSec> + <termSec> + <term>absorbtion nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa oscura</term> + </termSec> + <termSec> + <term>nebulosa de absorción</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c31"> + <note>G-Source: + http://mm04.nasaimages.org/MediaManager/srvr?mediafile=/Size3/NVA2-8-NA/14107/full_tif.jpg&userid=1&username=admin&resolution=3&servertype=JVA&cid=8&iid=NVA2&vcid=NA&usergroup=HUBBLE&profileid=39</note> + <langSec xml:lang="en"> + <termSec> + <term>reflection nebula</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>nebulosa de reflexión</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c32"> + <langSec xml:lang="en"> + <note>G-Source: http://nrumiano.free.fr/Images/Neutron_star_E.gif</note> + <termSec> + <term>neutron star</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <note>G-Source: + http://es.wikipedia.org/wiki/Archivo:Estrella_de_Neutrones.jpg</note> + <termSec> + <term>estrella de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c33"> + <langSec xml:lang="en"> + <note>For a star with no hydrogen content the limit is 1.44 solar masses, which + is thus the maximum possible for a white dwarf.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>Chandrasekhar limit</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>límite de Chandrasekhar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c34"> + <langSec xml:lang="en"> + <note>Encountered on in neutron stars.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>neutron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de neutrones</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c35"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>Schwarzschild radius</term> + <note>Related Term: event horizon</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>radio de Schwarzschild</term> + <note>Related Term: horizonte de sucesos, horizonte de eventos</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c36"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>event horizon</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>horizonte de sucesos</term> + </termSec> + <termSec> + <term>horizonte de eventos</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c37"> + <note>G-Source: http://en.wikipedia.org/wiki/File:FusionintheSun.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>proton-proton chain reaction</term> + </termSec> + <termSec> + <term>PP chain</term> + </termSec> + <termSec> + <term>proton-proton reaction</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>cadena protón-protón</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c38"> + <note>G-Source: http://en.wikipedia.org/wiki/File:CNO_Cycle.svg</note> + <langSec xml:lang="en"> + <termSec> + <term>carbon-nitrogen cycle</term> + </termSec> + <termSec> + <term>CNO cycle</term> + </termSec> + <termSec> + <term>carbon-nitrogen-oxygen cycle</term> + </termSec> + <termSec> + <term>Bethe-Weizsäcker-cycle</term> + </termSec> + <termSec> + <term>carbon cycle</term> + <note>The carbon cycle can also refer to the biogeochemical cycle by which + carbon is exchanged among the biosphere, pedosphere, geosphere, + hydrosphere, and atmosphere of the Earth.</note> + <note>N-Source: http://en.wikipedia.org/wiki/Carbon_cycle</note> + </termSec> + <termSec> + <term>CN cycle</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>ciclo CNO</term> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno-oxígeno</term> + </termSec> + <termSec> + <term>ciclo del carbono</term> + <note>También este término puede referirse a la formación de las moléculas + de carbohidratos, lípidos, proteínas y ácidos nucleicos.</note> + <note>N-Source: http://es.wikipedia.org/wiki/Ciclo_del_carbono</note> + </termSec> + <termSec> + <term>ciclo del carbono-nitrógeno</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c39"> + <langSec xml:lang="en"> + <termSec> + <term>degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c40"> + <langSec xml:lang="zu"> + <termSec> + <term>Oxford2003</term> + <note>Author[s]: Ridpath, Ian</note> + <note>Book Title: Astronomía</note> + <note>Publication Place: Spain</note> + <note>Publisher: Oxford University Press</note> + <note>Publication Year: 2003</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c41"> + <langSec xml:lang="en"> + <note>Electron degeneracy supports white dwarf stars against further + collapse.</note> + <note>N-Source: Oxford2007</note> + <termSec> + <term>electron degeneracy</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>degeneración de electrones</term> + </termSec> + <termSec> + <term>degeneración electrónica</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c42"> + <note>G-Source: + http://www.astro.cornell.edu/academics/courses/astro2201/images/bh_structure.gif</note> + <langSec xml:lang="en"> + <termSec> + <term>singularity</term> + <note>Related Term: black hole, event horizon, Schwarzschild radius</note> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>singularidad</term> + <note>Related Term: agujero negro, horizonte de sucesos, radio de + Schwarzschild</note> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c43"> + <note>G-Source: http://en.wikipedia.org/wiki/Solar_mass</note> + <note>In this graphic, the M with a subscript is the symbol for a solar mass.</note> + <note>N-Source: Jonathan Tomolonis</note> + <langSec xml:lang="en"> + <termSec> + <term>solar mass</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>masa solar</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c44"> + <note>G-Source: + http://upload.wikimedia.org/wikipedia/commons/thumb/5/5d/Triple-Alpha_Process.svg/750px-Triple-Alpha_Process.svg.png</note> + <langSec xml:lang="en"> + <termSec> + <term>triple-alpha process</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>proceso triple-alfa</term> + </termSec> + </langSec> + </conceptEntry> + <conceptEntry id="c45"> + <note>G-Source: + http://www.dorlingkindersley-uk.co.uk/static/clipart/uk/dk/sci_space/image_sci_space013.jpg</note> + <langSec xml:lang="en"> + <termSec> + <term>black dwarf</term> + </termSec> + </langSec> + <langSec xml:lang="es"> + <termSec> + <term>enana negra</term> + </termSec> + </langSec> + </conceptEntry> + </body> + <back> + <refObjectSec type="respPerson"> + <refObject id="pe324as3-9615-4d41-a9c8-30c36bffe0e6"> + <item type="fn">Tommy Tomolonis</item> + </refObject> + </refObjectSec> + </back> + </text> +</tbx>