Swift XRT/UVOT follow-up of the Black Hole Candidate MAXI J1659-152 during a low luminosity state
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| Publication date | 02-03-2011 |
| Journal | The astronomer's telegram |
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| Abstract | We report on a Swift follow-up observation of the X-ray transient MAXI J1659-152 (ATel #2873, ATel #2877, GCN #11296). This source is suggested to be a stellar-mass black hole candidate (Kalamkar et al. 2011, arXiv:1012.4330). The source also has a very short orbital period ~2.4 hours (Kuulkers et al. 2011, arXiv:1102.2102). The optical counterpart of MAXI J1659-152 has been identified (GCN #11298, ATel #2884), and the quiescent optical magnitude has been found to be 22.4 in r-band (ATel #2976). |
| Document type | Article |
| Language | English |
| Published at | https://www.astronomerstelegram.org/?read=3201 |
| Other links | https://ui.adsabs.harvard.edu/abs/2011ATel.3201....1Y/abstract |
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Swift XRT-UVOT follow-up of the Black Hole Candidate MAXI J1659-152 during a low luminosity state
(Final published version)
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