Variability Model for the Microquasar GRS 1915+105

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

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/906

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0004343
 http://arxiv.org/abs/astro-ph/0004343

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arXiv