X-ray Radio Correlation In Black Hole Sources
| dc.creator | Rao, A. R. | |
| dc.date | 2006-11-13 | |
| dc.date.accessioned | 2026-07-07T10:20:47Z | |
| dc.date.available | 2026-07-07T10:20:47Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611373 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611373 | |
| dc.identifier | PoSMQW6:010,2006 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/174962 | |
| dc.subject | Astrophysics | |
| dc.title | X-ray Radio Correlation In Black Hole Sources | |
| dc.type | text |