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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. 5.

Phase lags corresponding to two sets of light curves generated as described in the text. The light curves had the following parameters (1) ﹩\alpha =0.5﹩, ﹩\beta =16﹩ s, ﹩t_{0}=0.02﹩ s. (2) ﹩\alpha =0.55﹩, ﹩\beta =16﹩ s, ﹩t_{0}=0.02﹩ s. (3) ﹩\alpha =0.6﹩, ﹩\beta =16﹩ s, ﹩t_{0}=0.02﹩ s. The two curves correspond to the lags between (1)–(2) (solid line) and (1)–(3) (dotted line).

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