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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. 3.

Model light curves constructed using the prescription of eq. (6). Both curves use ﹩\alpha =0.5﹩, ﹩\gamma =1.5﹩, ﹩\beta =1.5﹩ s, ﹩t_{0}=0.001﹩ s, ﹩b=1﹩ but two different values of the mean arrival time between shots. The corresponding parameter f takes the values ﹩f=3﹩ (Fig. 3a) and ﹩f=10﹩ (Fig. 3b).
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