Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q16840332> ?p ?o }
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- Q16840332 subject Q10655.
- Q16840332 subject Q7824699.
- Q16840332 subject Q8691170.
- Q16840332 abstract "GRO J1719-24 (GRS 1716-249, V2293 Oph, X-Ray Nova Ophiuchi 1993) is supposed to be a low-mass X-ray binary. Its name derives from an X-ray transient, detected in 1993. The system consists of a black hole candidate and a low mass companion, estimated to be a main sequence star of the spectral type K05-V.The rotation period is uncertain, estimated at 14.7h. The light curve possibly exhibits some faster fluctuations as well, which are hypothesized to be produced by blobs of matter in the accretion disk.".
- Q16840332 wikiPageWikiLink Q1047034.
- Q16840332 wikiPageWikiLink Q10655.
- Q16840332 wikiPageWikiLink Q237604.
- Q16840332 wikiPageWikiLink Q3450.
- Q16840332 wikiPageWikiLink Q5961.
- Q16840332 wikiPageWikiLink Q675076.
- Q16840332 wikiPageWikiLink Q7824699.
- Q16840332 wikiPageWikiLink Q8041583.
- Q16840332 wikiPageWikiLink Q863936.
- Q16840332 wikiPageWikiLink Q8691170.
- Q16840332 type Place.
- Q16840332 type CelestialBody.
- Q16840332 type Location.
- Q16840332 type Place.
- Q16840332 type Star.
- Q16840332 type Thing.
- Q16840332 comment "GRO J1719-24 (GRS 1716-249, V2293 Oph, X-Ray Nova Ophiuchi 1993) is supposed to be a low-mass X-ray binary. Its name derives from an X-ray transient, detected in 1993. The system consists of a black hole candidate and a low mass companion, estimated to be a main sequence star of the spectral type K05-V.The rotation period is uncertain, estimated at 14.7h.".
- Q16840332 label "GRO J1719-24".
- Q16840332 name "GRO J1719-24".