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)

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