arXiv Analytics

Sign in

arXiv:1001.0676 [astro-ph.HE]AbstractReferencesReviewsResources

Spectral/timing evolution of black-hole binaries

Tomaso M. Belloni

Published 2010-01-05Version 1

I briefly outline the state-paradigm that has emerged from the study of black-hole binaries with RossiXTE. This is the starting point of a number of studies that address the connection between accretion and jet ejection and the physical nature of the hard spectral components in these systems.

Comments: 4 pages, 2 figures.To appear in Proceedings of "X-ray Astronomy 2009: Present Status, Multi-Wavelength Approach and Future Perspectives", Bologna, Italy, September 7-11, 2009, AIP, eds. A. Comastri, M. Cappi, and L. Angelini
Categories: astro-ph.HE
Related articles: Most relevant | Search more
arXiv:0909.2474 [astro-ph.HE] (Published 2009-09-14)
States and transitions in black-hole binaries
arXiv:1605.08351 [astro-ph.HE] (Published 2016-05-26)
'Spectro-temporal' variabilities and possible physical mechanism for Jet ejections
arXiv:0908.3077 [astro-ph.HE] (Published 2009-08-21)
Black-hole binaries: life begins at 40 keV

Links

Toolbox