Spectral components in black hole X-ray binaries
arXiv:1511.05887 · doi:10.1002/asna.201612319
Abstract
This paper summarises our current understanding of the spectral continuum components observed in black hole X-ray binaries. The consequences for theoretical models are discussed with an emphasis on the constraints set by observations on the nature of the X-ray corona in different spectral states.
7 pages, 3 figures, invited review at the XMM-Newton 2015 Science Workshop, The Extremes of Black Hole Accretion, ESAC, Madrid, Spain, 8th - 10th June 2015, accepted for publication in Astronomische Nachrichten
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Cited by in corpus (6)
- The 2015 Decay of the Black Hole X-ray Binary V404 Cygni: Robust Disk-Jet Coupling and a Sharp Transition into Quiescence
- The X-ray Polarization of the Accretion Disk Coronae of Active Galactic Nuclei
- Hard X-ray variability of V404 Cyg during the 2015 outburst
- The X/gamma-ray correlation in NGC 4945 and the nature of its gamma-ray source
- Radio & X-ray detections of GX 339--4 in quiescence using MeerKAT and Swift
- Radio/X-ray monitoring of the broad-line radio galaxy 3C 382. High-energy view with XMM-Newton and NuSTAR