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Modeling the Time Variability of Accreting Compact Sources

  • Authors: Demosthenes Kazanas and Xin-Min Hua

Kazanas & Hua 1999 The Astrophysical Journal 519 750.

  • Provider: AAS Journals

Caption: Fig. 1.

Response function a corona with ﹩p=1﹩ and ﹩r_{1}=6.35\times 10^{-3}\ \mathrm{lt}\,- \mathrm{s}\,=1.9\times 10^{8}﹩ cm, ﹩r_{2}=6.24\ \mathrm{lt}\,- \mathrm{s}\,=1.87\times 10^{11}﹩ cm, ﹩T_{e}=100﹩ keV, ﹩\tau _{0}=1﹩, and ﹩n_{1}=10^{15}﹩ cm−3 (long‐dashed curve) along with its fit by eq. (4) with ﹩\alpha =0.4﹩, ﹩\gamma =1.5﹩, ﹩\beta =10﹩ s, ﹩t_{0}=0.02﹩ s, ﹩b=1﹩ (solid curve), and the corresponding power spectrum (short‐dashed curve).

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