@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/226>
  skos:prefLabel "Chemically peculiar stars"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1025> .

<http://astrothesaurus.org/uat/995>
  skos:prefLabel "Magnetic stars"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1025> .

<http://astrothesaurus.org/uat/1025>
  dc:modified "2020-11-10T19:23:39.864Z"^^xsd:dateTime, "2020-11-10T19:23:49.915Z"^^xsd:dateTime ;
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie> ;
  skos:prefLabel "Mercury-manganese stars"@en ;
  a skos:Concept ;
  skos:broader <http://astrothesaurus.org/uat/995>, <http://astrothesaurus.org/uat/128>, <http://astrothesaurus.org/uat/226> ;
  skos:editorialNote [ ] ;
  skos:altLabel "Mercury manganese stars"@en ;
  skos:definition "Chemically peculiar stars of late B-types. The most distinctive features of Mercury-manganese stars are extreme atmospheric overabundance of Hg (up to 5 dex) and of Mn (up to 3 dex). The origin of abundance anomalies observed in late B-type stars with HgMn peculiarity is still poorly understood. More than two thirds of the HgMn stars are known to belong to spectroscopic binaries with a preference of orbital periods ranging from 3 to 20 days."@en .

<http://astrothesaurus.org/uat/128>
  skos:prefLabel "B stars"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1025> .