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GRS 1915+105 and the disc-jet coupling in accreting black hole systems

GRS 1915+105 and the disc-jet coupling in accreting black hole systems
GRS 1915+105 and the disc-jet coupling in accreting black hole systems
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.
317-364
Fender, Rob
c802ddfc-25a3-4c0e-899d-11c405c705d1
Belloni, Tomaso
55fb4c9b-fe03-4af0-bd02-201635b1ea20
Fender, Rob
c802ddfc-25a3-4c0e-899d-11c405c705d1
Belloni, Tomaso
55fb4c9b-fe03-4af0-bd02-201635b1ea20

Fender, Rob and Belloni, Tomaso (2004) GRS 1915+105 and the disc-jet coupling in accreting black hole systems. Annual Reviews of Astronomy and Astrophysics, 42, 317-364. (doi:10.1146/annurev.astro.42.053102.134031).

Record type: Article

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.

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More information

Published date: September 2004
Additional Information: First published online as a Review in Advance on June 1, 2004

Identifiers

Local EPrints ID: 40537
URI: http://eprints.soton.ac.uk/id/eprint/40537
PURE UUID: 18936de8-4b63-4306-9b41-f1a65294156f

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Date deposited: 03 Jul 2006
Last modified: 15 Mar 2024 08:20

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Contributors

Author: Rob Fender
Author: Tomaso Belloni

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