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

doi:10.1111/j.1365-2966.2005.09843.x

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

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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 and Walter H. G. Lewin

Monthly Notices of the Royal Astronomical Society, Vol.366(1), pp.235-237

02/2006

DOI: https://doi.org/10.1111/j.1365-2966.2005.09843.x

Abstract

Stars: individual: XTE J1650-500

X-rays: stars

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 (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). © 2005 RAS.

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Title: XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence
Creators - without role: Jeroen Homan - MIT , Kavli Institute for Astrophysics and Space Research
Rudy Wijnands - University of Amsterdam
Albert Kong - MIT , Kavli Institute for Astrophysics and Space Research
Jon M. Miller - University of Michigan
Sabrina Rossi - Brera Astronomical Observatory
Tomaso Belloni - Brera Astronomical Observatory
Walter H. G. Lewin - MIT , Kavli Institute for Astrophysics and Space Research
Publication Details: Monthly Notices of the Royal Astronomical Society, Vol.366(1), pp.235-237
Identifiers: 9957769138106774
Academic Unit: Institute of Astronomy, College of Science, National Tsing Hua University
Language: English
Resource Type: Journal article

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

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