XMM–Newton observations of the black hole X-ray transient XTE J1650–500 in quiescence
dc.contributor.author | Homan, Jeroen | en_US |
dc.contributor.author | Wijnands, Rudy | en_US |
dc.contributor.author | Kong, Albert | en_US |
dc.contributor.author | Miller, Jon M. | en_US |
dc.contributor.author | Rossi, Sabrina | en_US |
dc.contributor.author | Belloni, Tomaso | en_US |
dc.contributor.author | Lewin, Walter H. G. | en_US |
dc.date.accessioned | 2010-06-01T18:27:43Z | |
dc.date.available | 2010-06-01T18:27:43Z | |
dc.date.issued | 2006-02 | en_US |
dc.identifier.citation | Homan, Jeroen; Wijnands, Rudy; Kong, Albert; Miller, Jon M.; Rossi, Sabrina; Belloni, Tomaso; Lewin, Walter H. G. (2006). " XMM–Newton observations of the black hole X-ray transient XTE J1650–500 in quiescence." Monthly Notices of the Royal Astronomical Society 366(1): 235-237. <http://hdl.handle.net/2027.42/71669> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/71669 | |
dc.description.abstract | We report the result of an XMM–Newton observation of the black hole X-ray transient XTE J1650–500 in quiescence. The source was not detected, and we set upper limits on the 0.5–10 keV luminosity of 0.9–1.0 × 10 31 erg s −1 (for a newly derived distance of 2.6 kpc). These limits are in line with the quiescent luminosities of black hole X-ray binaries with similar orbital periods (∼7–8 h). | en_US |
dc.format.extent | 60116 bytes | |
dc.format.extent | 3109 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.publisher | Blackwell Science Ltd | en_US |
dc.rights | 2005 The Authors. Journal compilation © 2005 RAS | en_US |
dc.subject.other | Stars: Individual: XTE J1650–500 | en_US |
dc.subject.other | X-rays: Stars | en_US |
dc.title | XMM–Newton observations of the black hole X-ray transient XTE J1650–500 in quiescence | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | The University of Michigan, 500 Church Street, Dennison 814, Ann Arbor, MI 48109-1042, USA | en_US |
dc.contributor.affiliationother | MIT Kavli Institute for Astrophysics and Space Research, 70 Vassar Street, Cambridge, MA 02139, USA | en_US |
dc.contributor.affiliationother | Astronomical Institute ‘Anton Pannekoek’, University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, the Netherlands | en_US |
dc.contributor.affiliationother | INAF Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/71669/1/j.1365-2966.2005.09843.x.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2005.09843.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
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dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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