Physical Characteristics of the Spectral States of Galactic Black Holes
arXiv:astro-ph/9707244 · doi:10.1063/1.53969
Abstract
Using simple analytical estimates we show how the physical parameters characterizing different spectral states of the galactic black hole candidates can be determined using spectral data presently available.
arXiv comment5 pages, 3 figures, to appear in the Proceedings of 4th Compton Symposium, April 27-30, 1997, Williamsburg, Virginia, USA