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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. 4.

Two composite PDSs: EXOSAT spectra with matching HF PCA PDS. PCA data for the lower PDS are taken from observation ID 40099‐01‐03‐01 and for the upper PDS from observation ID 40099‐01‐05‐00. Data are fitted by an LF‐HF diffusion model: ﹩\chi ^{2}/ N_{\mathrm{dof}\,}=250.1/ 267=0.94﹩, ﹩\psi _{\mathrm{cor}\,}=2.32\pm 0.12﹩, ﹩t_{0,C}=1.8\pm 0.3﹩, ﹩\psi _{D}=2.5﹩ (fixed) and ﹩\chi ^{2}/ N_{\mathrm{dof}\,}=278.5/ 267=1.04﹩, ﹩\psi _{\mathrm{cor}\,}=2.07\pm 0.7﹩, ﹩t_{0,C}=1.24\pm 0.12﹩, ﹩\psi _{D}=0.3\pm 0.3﹩ (fixed) for lower and upper fits, respectively.

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