Английская Википедия:GRO J1719-24

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GRO J1719-24 (GRS 1716-249, V2293 Oph, X-Ray Nova Ophiuchi 1993) is believed to be a low-mass X-ray binary.[1] Its name derives from an X-ray transient, detected in 1993.[2] The system consists of a black hole candidate and a low mass companion, estimated to be a main sequence star of the spectral type K0-5 V.[3]

The rotation period is uncertain, estimated at 14.7h.[4] The light curve possibly exhibits some faster fluctuations as well, which are hypothesized to be produced by blobs of matter in the accretion disk.[4]

References

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  4. 4,0 4,1 Ошибка цитирования Неверный тег <ref>; для сносок Masetti1996 не указан текст