Fig. 3 from 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

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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. 3.

Same as Fig. 2, but for observations 50109‐01‐01‐00 (top) and 60090‐01‐14‐01 (bottom). The first observation is taken during the intermediate state just before the transition to the high‐soft state, which is presented by the second observation. No HF WRN is present in PDS during the high‐soft state.

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