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XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence

Jeroen Homan·Rudy Wijnands·Albert Kong·Jon M. Miller·Sabrina Rossi·Tomaso Belloni·Walter H. G. Lewin
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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 0.9e31-1.0e31 erg/s (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 hr)

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Jeroen Homan, Rudy Wijnands, Albert Kong, Jon M. Miller, Sabrina Rossi, Tomaso Belloni, Walter H. G. Lewin. 2005-11-17. XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence. https://doi.org/10.1111/j.1365-2966.2005.09843.x

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