Figure 10 from Spectral Index as a Function of Mass Accretion Rate in Black Hole Sources: Monte Carlo Simulations and an Analytical Description

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Spectral Index as a Function of Mass Accretion Rate in Black Hole Sources: Monte Carlo Simulations and an Analytical Description

Authors: Philippe Laurent and Lev Titarchuk

Laurent & Titarchuk 2011 The Astrophysical Journal 727 34.

Provider: AAS Journals

Caption: Figure 10.

Index vs. in the presence of sub-Keplerian flow above the disk. The accretion flow has the same electron temperature as the TL one. The ratio of . Total

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