@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/1781>
  skos:prefLabel "von Zeipel theorem"@en ;
  a skos:Concept ;
  skos:related <http://astrothesaurus.org/uat/1629> .

<http://astrothesaurus.org/uat/1334>
  skos:prefLabel "Radiative braking"@en ;
  a skos:Concept ;
  skos:broader <http://astrothesaurus.org/uat/1629> .

<http://astrothesaurus.org/uat/1624>
  skos:prefLabel "Stellar properties"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1629> .

<http://astrothesaurus.org/uat/1629>
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie>, <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin> ;
  skos:related <http://astrothesaurus.org/uat/1524>, <http://astrothesaurus.org/uat/1781> ;
  skos:narrower <http://astrothesaurus.org/uat/1334>, <http://astrothesaurus.org/uat/680> ;
  skos:prefLabel "Stellar rotation"@en ;
  a skos:Concept ;
  dc:modified "2020-11-24T17:24:35.632Z"^^xsd:dateTime, "2020-11-19T16:21:21.675Z"^^xsd:dateTime ;
  skos:broader <http://astrothesaurus.org/uat/1624> ;
  skos:definition "The spinning of a star about its axis, due to its angular momentum. Stars do not necessarily rotate as solid bodies, and their angular momentum may be distributed non-uniformly, depending on radius or latitude. Thus the equator of the star can rotate at a different angular velocity than the higher latitudes. These differences in the rate of rotation within a star may have a significant role in the generation of a stellar magnetic field."@en ;
  skos:editorialNote [ ] .

<http://astrothesaurus.org/uat/680>
  skos:prefLabel "Gravity darkening"@en ;
  a skos:Concept ;
  skos:broader <http://astrothesaurus.org/uat/1629> .

<http://astrothesaurus.org/uat/1524>
  skos:prefLabel "Solar rotation"@en ;
  a skos:Concept ;
  skos:related <http://astrothesaurus.org/uat/1629> .