2000/12/29 by Anuj Nandi, Sivakumar G. Manickam, Sandip K. Chakrabarti
Physics and Astronomy · #astro-ph
published as Indian Journal of Physics, 74(B) No. 5, p. 331 · Latex file with two figures
arxiv created 2000/12/29 · arxiv updated 2009/12/01
The black hole candidate GRS 1915+105 exhibits a rich variety of variability. Assuming that the earlier paradigm of black hole accretion which includes a shock is applicable for this system as well, one can classify these variabilities into four classes. We present light curves of these classes and discuss the basis of our classification.