Variability Model for the Microquasar GRS 1915+105

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dc.creatorJaniuk, Agnieszka
dc.creatorCzerny, Bozena
dc.creatorSiemiginowska, Aneta
dc.creatorAbramowicz, Marek A.
dc.date2000-04-25
dc.date.accessioned2026-07-07T01:53:16Z
dc.date.available2026-07-07T01:53:16Z
dc.descriptionWe 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.
dc.description5 pages, 2 postscript figures; contribution to the conference "DISCS 2000", Kopenhagen, January 5-8 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0004343
dc.identifierhttp://arxiv.org/abs/astro-ph/0004343
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/906
dc.subjectAstrophysics
dc.titleVariability Model for the Microquasar GRS 1915+105
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