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XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence
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 × 1031 erg s−1 (for a newly derived distance of 2.6 kpc). These limits are in line with the qu...
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Published in: | Monthly notices of the Royal Astronomical Society 2006-02, Vol.366 (1), p.235-237 |
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container_title | Monthly notices of the Royal Astronomical Society |
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creator | Homan, Jeroen Wijnands, Rudy Kong, Albert Miller, Jon M. Rossi, Sabrina Belloni, Tomaso Lewin, Walter H. G. |
description | 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 × 1031 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). |
doi_str_mv | 10.1111/j.1365-2966.2005.09843.x |
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source | Oxford Journals Open Access Collection; EZB Electronic Journals Library |
subjects | Black holes Luminosity stars: individual: XTE J1650-500 X-ray astronomy X-rays: stars |
title | XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence |
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