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Power Spectra of Black Holes and Neutron Stars as a Probe of Hydrodynamic Structure of the Source: Diffusion Theory and Its Application to Cygnus X‐1 and Cygnus X‐2 X‐Ray Observations

  • Authors: Lev Titarchuk, Nikolai Shaposhnikov, and Vadim Arefiev

Titarchuk, Shaposhnikov, & Arefiev 2007 The Astrophysical Journal 660 556.

  • Provider: AAS Journals

Caption: Fig. 7.

Cyg X‐1: HF photon diffusion PDS (Lorentzian): the best‐fit photon diffusion time ﹩t_{*}﹩ vs. photon index Γ.

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