{ "d" : { "results": [ { "__metadata": { "uri": "http://dbpedia.org/resource/V_Coronae_Australis" }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Var-star-stub" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/International_Celestial_Reference_System" } }, "http://www.w3.org/2002/07/owl#sameAs": { "__deferred": { "uri": "http://www.wikidata.org/entity/Q18210648" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Corona_Australis" } }, "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Durchmusterung_objects" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Cordoba_Durchmusterung" } }, "http://www.w3.org/1999/02/22-rdf-syntax-ns#type": { "__deferred": { "uri": "http://schema.org/Place" } }, "http://purl.org/linguistics/gold/hypernym": { "__deferred": { "uri": "http://dbpedia.org/resource/Star" } }, "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Carbon_stars" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Photometric_system" } }, "http://xmlns.com/foaf/0.1/name": "V Coronae Australis", "http://www.w3.org/1999/02/22-rdf-syntax-ns#type": { "__deferred": { "uri": "http://dbpedia.org/ontology/Star" } }, "http://dbpedia.org/property/temperature": "6250", "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Carbon_stars" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Henry_Draper_Catalogue" } }, "http://dbpedia.org/property/pError": "2.95", "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Henry_Draper_Catalogue_objects" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Stars_of_Corona_Australis" } }, "http://dbpedia.org/property/constell": { "__deferred": { "uri": "http://dbpedia.org/resource/Corona_Australis" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/File:VCrALightCurve.png" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_image" } }, "http://dbpedia.org/ontology/abstract": "V Coronae Australis (V CrA) is a R Coronae Borealis variable star in the constellation Corona Australis. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. V Coronae Australis dimmed in brightness from 1994 to 1998. It has around 60% the mass of the Sun and an effective (surface) temperature of around 6250 K.", "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_catalog" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_end" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Short_description" } }, "http://www.w3.org/2002/07/owl#sameAs": { "__deferred": { "uri": "https://global.dbpedia.org/id/kqeb" } }, "http://dbpedia.org/property/equinox": "J2000.0", "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_character" } }, "http://dbpedia.org/property/type": { "__deferred": { "uri": "http://dbpedia.org/resource/R_Coronae_Borealis_variable" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_astrometry" } }, "http://www.w3.org/1999/02/22-rdf-syntax-ns#type": { "__deferred": { "uri": "http://dbpedia.org/ontology/CelestialBody" } }, "http://xmlns.com/foaf/0.1/isPrimaryTopicOf": { "__deferred": { "uri": "http://en.wikipedia.org/wiki/V_Coronae_Australis" } }, "http://www.w3.org/1999/02/22-rdf-syntax-ns#type": { "__deferred": { "uri": "http://dbpedia.org/ontology/Place" } }, "http://dbpedia.org/property/propMoRa": "-0.9", "http://dbpedia.org/property/parallax": "-0.39", "http://www.w3.org/1999/02/22-rdf-syntax-ns#type": { "__deferred": { "uri": "http://www.w3.org/2002/07/owl#Thing" } }, "http://www.w3.org/2000/01/rdf-schema#comment": "V Coronae Australis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Södra kronan. Stjärnan har visuell magnitud +9,4 och når i förmörkelsefasen ner till +17,9. V Coronae Australis observerades i förmörkelsefasen från 1994 till 1998.", "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Reflist" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_detail" } }, "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Henry_Draper_Catalogue_objects" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:DEC" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Light_curve" } }, "http://dbpedia.org/property/mass": "0.6", "http://xmlns.com/foaf/0.1/depiction": { "__deferred": { "uri": "http://commons.wikimedia.org/wiki/Special:FilePath/VCrALightCurve.png" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Durchmusterung_objects" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_begin" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Variable_star_designation" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Objects_with_variable_star_designations" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_observe" } }, "http://www.w3.org/2002/07/owl#sameAs": { "__deferred": { "uri": "http://yago-knowledge.org/resource/V_Coronae_Australis" } }, "http://dbpedia.org/ontology/thumbnail": { "__deferred": { "uri": "http://commons.wikimedia.org/wiki/Special:FilePath/VCrALightCurve.png?width=300" } }, "http://www.w3.org/2000/01/rdf-schema#label": "V Coronae Australis", "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:R_Coronae_Borealis_variables" } }, "http://dbpedia.org/ontology/abstract": "V Coronae Australis är en eruptiv variabel av RCB-typ (RCB) i stjärnbilden Södra kronan. Stjärnan har visuell magnitud +9,4 och når i förmörkelsefasen ner till +17,9. V Coronae Australis observerades i förmörkelsefasen från 1994 till 1998.", "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Objects_with_variable_star_designations" } }, "http://www.w3.org/ns/prov#wasDerivedFrom": { "__deferred": { "uri": "http://en.wikipedia.org/wiki/V_Coronae_Australis?oldid=1060219061&ns=0" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/J2000.0" } }, "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Corona_Australis" } }, "http://dbpedia.org/ontology/wikiPageLength": "3908", "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:RA" } }, "http://dbpedia.org/ontology/wikiPageID": "43289315", "http://www.w3.org/2002/07/owl#sameAs": { "__deferred": { "uri": "http://sv.dbpedia.org/resource/V_Coronae_Australis" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Hipparcos_objects" } }, "http://www.w3.org/2000/01/rdf-schema#comment": "V Coronae Australis (V CrA) is a R Coronae Borealis variable star in the constellation Corona Australis. These are extremely hydrogen-deficient supergiants thought to have arisen as the result of the merger of two white dwarfs; fewer than 100 have been discovered as of 2012. V Coronae Australis dimmed in brightness from 1994 to 1998. It has around 60% the mass of the Sun and an effective (surface) temperature of around 6250 K.", "http://dbpedia.org/property/propMoDec": "-3.83", "http://www.w3.org/1999/02/22-rdf-syntax-ns#type": { "__deferred": { "uri": "http://dbpedia.org/ontology/Location" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Hipparcos" } }, "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Hipparcos_objects" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Constellation" } }, "http://www.w3.org/2002/07/owl#sameAs": { "__deferred": { "uri": "http://rdf.freebase.com/ns/m.0115lg19" } }, "http://dbpedia.org/ontology/wikiPageRevisionID": "1060219061", "http://purl.org/dc/terms/subject": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:R_Coronae_Borealis_variables" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/R_Coronae_Borealis_variable" } }, "http://dbpedia.org/property/wikiPageUsesTemplate": { "__deferred": { "uri": "http://dbpedia.org/resource/Template:Starbox_reference" } }, "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Effective_temperature" } }, "http://www.w3.org/2000/01/rdf-schema#label": "V Coronae Australis", "http://dbpedia.org/ontology/wikiPageWikiLink": { "__deferred": { "uri": "http://dbpedia.org/resource/Category:Corona_Australis" } }, "http://dbpedia.org/property/epoch": { "__deferred": { "uri": "http://dbpedia.org/resource/J2000.0" } } } ], "__count": "1" } }