X-ray Radio Correlation In Black Hole Sources
Abstract
We examine the X-ray - radio correlation in Galactic black hole sources. We highlight some of the results which extend the flux-flux relations to sources with very high accretion rates. Some of the recent results indicate that the synchrotron process is unlikely to be the mechanism responsible for the X-ray emission, particularly at high accretion rates. We present a truncated accretion disk scenario and argue that accretion rate and accretion disk geometry ultimately act as a driver of the X-ray - radio correlation. We stress the importance of wide-band X-ray spectral measurements to understand the disk-jet connection and briefly outline some attempts made in the Indian context to build instruments for wide-band X-ray spectroscopy.
Keywords
Cite
@article{arxiv.astro-ph/0611373,
title = {X-ray Radio Correlation In Black Hole Sources},
author = {A. R. Rao},
journal= {arXiv preprint arXiv:astro-ph/0611373},
year = {2008}
}
Comments
11 pages, 5 figures; accepted for publication in the proceedings of VI Microquasar Workshop: Microquasars and Beyond, 18-22 September 2006, Como (Italy), ed: T. Belloni (2006)