Fundamental States of Accretion/Jet Configuration and the Black Hole Candidate GRS1915+105
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Advective 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.
Latex file and four figures. Indian Journal of Physics (in press)
Latex file and four figures. Indian Journal of Physics (in press)