@prefix skos: <http://www.w3.org/2004/02/skos/core#> .
@prefix dc: <http://purl.org/dc/terms/> .
@prefix xsd: <http://www.w3.org/2001/XMLSchema#> .

<http://astrothesaurus.org/uat/108>
  skos:related <http://astrothesaurus.org/uat/2100> ;
  a skos:Concept ;
  skos:prefLabel "Asymptotic giant branch"@en ;
  skos:altLabel "AGB"@en ;
  dc:modified "2020-11-05T18:59:52.888Z"^^xsd:dateTime, "2020-11-09T21:28:43.36Z"^^xsd:dateTime ;
  skos:broader <http://astrothesaurus.org/uat/725> ;
  skos:editorialNote [ ] ;
  skos:definition "A region of the Hertzsprung-Russell diagram populated by evolving low-mass to intermediate-mass stars. These stars have an electron degenerate core of carbon and oxygen surrounded by two burning shells of helium and hydrogen. The H and He-burning shells are activated alternately in the deep layers of the star. An extended and tenuous convection envelope, having a radius of 10^4 - 10^5 times the size of the core, lies above these shells. The loosely bound envelope is gradually eroded by the strong stellar wind, which forms a dusty circumstellar envelope out to several hundreds of stellar radii. The convective envelope, stellar atmosphere, and circumstellar envelope have a rich and changing chemical composition provided by nucleosynthesis processes in the burning shells in the deep interior."@en ;
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin> .

<http://astrothesaurus.org/uat/2100>
  skos:prefLabel "Asymptotic giant branch stars"@en ;
  a skos:Concept ;
  skos:related <http://astrothesaurus.org/uat/108> .

<http://astrothesaurus.org/uat/725>
  skos:prefLabel "Hertzsprung Russell diagram"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/108> .

