Fundamental States of Accretion/Jet Configuration and the Black Hole Candidate GRS1915+105

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dc.creatorChakrabarti, Sandip K.
dc.creatorNandi, Anuj
dc.date2000-12-29
dc.date.accessioned2026-07-07T01:57:12Z
dc.date.available2026-07-07T01:57:12Z
dc.descriptionAdvective disk paradigm of black hole accretion includes self-consistent formation of shocks and outflows from post-shock region. We apply this paradigm to understand rich variation of the light curve of the black hole candidate GRS1915+105. We propose that out of five possible {\it fundamental states} the black hole candidate GRS1915+105 moves around among three of them creating all possible observed light curves.
dc.descriptionLatex file and four figures. Indian Journal of Physics (in press)
dc.identifierhttps://arxiv.org/abs/astro-ph/0012526
dc.identifierhttp://arxiv.org/abs/astro-ph/0012526
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2290
dc.subjectAstrophysics
dc.titleFundamental States of Accretion/Jet Configuration and the Black Hole Candidate GRS1915+105
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