GRS 1915+105 and the Disc-Jet Coupling in Accreting Black Hole Systems
| dc.creator | Fender, Rob | |
| dc.creator | Belloni, Tomaso | |
| dc.date | 2004-06-22 | |
| dc.date | 2004-06-23 | |
| dc.date.accessioned | 2026-07-07T10:47:52Z | |
| dc.date.available | 2026-07-07T10:47:52Z | |
| dc.description | GRS 1915+105 - the first stellar-scale, highly relativistic jet source identified - is a key system for our understanding of the disc-jet coupling in accreting black hole systems. Comprehending the coupling between inflow and outflow in this source is important not only for X-ray binary systems but has a broader relevance for studies of active galactic nuclei and gamma-ray bursts. In this paper, we present a detailed review of the observational properties of the system, as established in the decade since its discovery. We attempt to place it in context by a detailed comparison with other sources, and construct a simple model for the disc-jet coupling, which may be more widely applicable to accreting black hole systems. | |
| dc.description | Annual Reviews of Astronomy and Astrophysics, in press. Some typos corrected and Fig 27 replaced with correct version | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0406483 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0406483 | |
| dc.identifier | Ann.Rev.Astron.Astrophys.42:317-364,2004 | |
| dc.identifier | doi:10.1146/annurev.astro.42.053102.134031 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183686 | |
| dc.subject | Astrophysics | |
| dc.title | GRS 1915+105 and the Disc-Jet Coupling in Accreting Black Hole Systems | |
| dc.type | text |