Автор |
Fender, Rob |
Автор |
Belloni, Tomaso |
Дата выпуска |
2004 |
dc.description |
▪ Abstract 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 not only is important 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. |
Формат |
application.pdf |
Издатель |
Annual Reviews |
Копирайт |
Annual Reviews |
Название |
GRS 1915+105 AND THE DISC-JET COUPLING IN ACCRETING BLACK HOLE SYSTEMS |
DOI |
10.1146/annurev.astro.42.053102.134031 |
Print ISSN |
0066-4146 |
Журнал |
Annual Review of Astronomy and Astrophysics |
Том |
42 |
Первая страница |
317 |
Последняя страница |
364 |
Аффилиация |
Fender, Rob; Astronomical Institute Anton Pannekoek, University of Amsterdam , Kruislaan 403, 1098 SJ Amsterdam , The Netherlands |