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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

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