Variability Model for the Microquasar GRS 1915+105

Details Variability Model for the Microquasar GRS 1915+105 Variability Model for the Microquasar GRS 1915+105

2000-04-25

arxiv.org/abs/astro-ph/0004343v1

Astronomy and Astrophysics

Astrophysics

5 pages, 2 postscript figures; contribution to the conference "DISCS 2000", Kopenhagen, January 5-8 2000

Scientific paper

We analyse the radiation pressure instability of the standard, optically
thisc disc and propose it as an explanation of the obseved variability of the
superluminal microquasar GRS 1915+105. The quantitave agreement with the
observed outburst amplitudes is obtained under the assumption that substantial
part of the energy is carried away by the jet.

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