{ "format" : "linked-data-api", "version" : "0.2", "result" : {"_about" : "https://vocabs.ardc.edu.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/5-1-0/resource.text?uri=http%3A%2F%2Fastrothesaurus.org%2Fuat%2F276", "definition" : "https://vocabs.ardc.edu.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/5-1-0/resource.text?uri=http%3A%2F%2Fastrothesaurus.org%2Fuat%2F276", "extendedMetadataVersion" : "https://vocabs.ardc.edu.au/repository/api/lda/aas/the-unified-astronomy-thesaurus/5-1-0/resource.text?_metadata=all&uri=http%3A%2F%2Fastrothesaurus.org%2Fuat%2F276", "primaryTopic" : {"_about" : "http://astrothesaurus.org/uat/276", "broader" : [{"_about" : "http://astrothesaurus.org/uat/352", "narrower" : ["http://astrothesaurus.org/uat/276"]}
      ], "contributor" : "http://editor.vocabs.ands.org.au/user/AAS_Frey.Katie_Admin", "dctermsModified" : "Thu, 05 Nov 2020 15:36:05 GMT+0000", "definition" : "A relatively small cloud of dust and gas in the interstellar medium shaped like a comet with a bright-rimmed head. Cometary globules are situated near young massive stars with a strong stellar wind. The wind ionizes gases on the side facing the O stars and sweep away the low-density gas toward the tail. Cometary globules are believed to be molecular cloud condensations, which are so dense that they are not disrupted when an H II region expands into the molecular cloud surrounding it. The Rosette nebula is a good example of an H II region which shows an abundance of cometary globules.", "prefLabel" : {"_value" : "Cometary globules", "_lang" : "en"}
      , "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"]}
}