2000/12/29 by Sandip K. Chakrabarti, Anuj Nandi, Chakrabarti, Sandip K. +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0012526
Latex file and four figures. Indian Journal of Physics (in press)
arxiv created 2000/12/29 · arxiv updated 2009/12/01
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.