{ "format" : "linked-data-api", "version" : "0.2", "result" : {"_about" : "http://vocabs.ands.org.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/3-1-0/resource.text?uri=http://astrothesaurus.org/uat/2045", "definition" : "http://vocabs.ands.org.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/3-1-0/resource.text?uri=http://astrothesaurus.org/uat/2045", "extendedMetadataVersion" : "http://vocabs.ands.org.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/3-1-0/resource.text?_metadata=all&uri=http://astrothesaurus.org/uat/2045", "primaryTopic" : {"_about" : "http://astrothesaurus.org/uat/2045", "altLabel" : [{"_value" : "Chandrasekhar-Schonberg limit", "_lang" : "en"}
      , {"_value" : "Schoenberg-Chandrasekhar limit", "_lang" : "en"}
      ], "broader" : [{"_about" : "http://astrothesaurus.org/uat/662", "narrower" : ["http://astrothesaurus.org/uat/2045"]}
      ], "contributor" : "http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie", "creator" : "http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie", "dctermsCreated" : "Mon, 10 Sep 2018 16:07:43 GMT+0000", "dctermsModified" : "Tue, 11 Sep 2018 18:40:36 GMT+0000", "definition" : "This represents the maximum fraction of a star's mass that can be contained within an isothermal core while still supporting the rest of the star in hydrostatic equilibrium.  Once the mass of an isothermal helium core exceeds this limit, the corse collapses and the star evolve rapidly.  The limit varies depending on the star.", "prefLabel" : {"_value" : "Schonberg-Chandrasekhar limit", "_lang" : "en"}
      , "related" : [{"_about" : "http://astrothesaurus.org/uat/1599", "related" : ["http://astrothesaurus.org/uat/2045"]}
      ], "scopeNote" : "Not to be confused with the Chandrasekhar limit.", "type" : ["http://www.w3.org/2000/01/rdf-schema#Resource", "http://www.w3.org/2004/02/skos/core#Concept"]}
    , "type" : ["http://purl.org/linked-data/api/vocab#ItemEndpoint", "http://purl.org/linked-data/api/vocab#Page"]}
}