@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/1625>
  skos:prefLabel "Stellar pulsations"@en ;
  a skos:Concept ;
  skos:narrower <http://astrothesaurus.org/uat/1309> .

<http://astrothesaurus.org/uat/1309>
  skos:editorialNote [ ] ;
  dc:contributor <http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin> ;
  skos:broader <http://astrothesaurus.org/uat/1625> ;
  skos:prefLabel "Pulsation modes"@en ;
  skos:definition "The way in which pulsations occur in a star due to the fact that stars act as resonant cavities, as studied in asteroseismology. A star may pulsate either with approximately spherical symmetry (radial pulsation), or as a series of waves running across the surface (non-radial pulsation). Pulsation may occur in a single mode or in multiple modes, depending on the type of star. Three different modes of pulsations have been detected through the helioseismology of the Sun: p mode, g mode, and f mode, generated by acoustic, gravity, and surface gravity waves respectively."@en ;
  dc:modified "2020-11-03T20:47:01.486Z"^^xsd:dateTime, "2020-11-03T20:46:46.623Z"^^xsd:dateTime ;
  a skos:Concept .