The Spectral Energy Distribution of Quiescent Black Hole X-Ray Binaries: New Constraints from Spitzer

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The Spectral Energy Distribution of Quiescent Black Hole X-Ray Binaries: New Constraints from Spitzer

Among the various issues that remain open in the field of accretion onto black hole X-ray binaries (BHBs) is the question of how gas accretes at very low Eddington ratios, in the so-called quiescent regime. While there is general agreement that X-rays are produced by a population of high-energy elec...

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Bibliographic Details
Main Authors:	Gallo, E., Migliari, S., Markoff, S., Tomsick, J., Bailyn, C., Berta, S., Fender, R., Miller-Jones, James
Format:	Journal Article
Published:	Institute of Physics Publishing, Inc. 2007
Subjects:	Radiation Mechanisms: General stars: individual (V404 Cyg) X-Rays: Binaries Stars: Individual: Alphanumeric: XTE J1118+480 Stars: Individual: Alphanumeric: A0620-00
Online Access:	http://iopscience.iop.org/0004-637X/670/1/600/ http://hdl.handle.net/20.500.11937/45780

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