Journal
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS
Volume 132, Issue -, Pages 337-345Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.nuclphysbps.2004.04.061
Keywords
-
Categories
Ask authors/readers for more resources
Our knowledge of the high-energy emission spectra from black-hole candidates has increased enormously with missions like BeppoSAX and KossiXTE, 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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available