High-Energy Spectra from Black-Hole Candidates
arXiv:astro-ph/0309028 · doi:10.1016/j.nuclphysbps.2004.04.061
Abstract
Our knowledge of the high-energy emission spectra from black-hole candidates has increased enormously with missions like BeppoSAX and RossiXTE, thanks to their broad-band window. I present the main and most solid points of this current knowledge, both in terms of detailed spectral modeling of X-ray broad-band spectra, and more generally in relation to the "black-hole state paradigm", which links spectral and timing properties of accretion disks. Finally, through the discussion of recent results on two systems, XTE J1650-500 and GX 339-4, I present evidence for a new view of the state paradigm.
9 pages, 11 figures, invited paper at the symposium: The Restless High-Energy Universe, Amsterdam, May 2003
References in corpus (6)
- Radio / X-ray correlation in the low/hard state of GX 339--4
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- The ABC of low-frequency quasi-periodic oscillations in Black-Hole Candidates: analogies with Z-sources
- A Global Spectral Study of Black Hole X-ray Binaries
- Long Term Variability of Cygnus X-1. IV. Spectral Evolution 1999-2004
- On the variation of black hole accretion disc radii as a function of state and accretion rate
- Time-dependent models of two-phase accretion discs around black holes
- Studying the X-ray hysteresis in GX 339-4: the disc and iron line over one decade
- Power-Colours: Simple X-ray Binary Variability Comparison
- On the X-ray spectra of luminous, inhomogeneous accretion flows
- Chandra X-Ray Spectroscopy of the Focused Wind in the Cygnus X-1 System. II. The Nondip Spectrum in the Low/Hard State - Modulations with Orbital Phase
- Hard X-ray variability of V404 Cyg during the 2015 outburst
- Combining timing characteristics with physical broadband spectral modelling of black hole X-ray binary GX~3394
- Constraining distance and inclination angle of V4641 Sgr using and observations during low soft spectral state
- Hunting the nature of IGR J17497-2821 with X-ray and NIR observations
- A disk-corona model for low/hard state of black hole X-ray binaries