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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. 6.

(a) Autocorrelation function computed using the corona response function g(t) (eq. [7]) with ﹩\alpha =0.38﹩, ﹩\beta =10﹩ s, and ﹩t_{0}=0.02﹩ s. (b) The autocorrelation function computed from a model light curve, generated according to eq. (6) with g(t) as above. (c) Same as in (a) plotted in logarithmic time coordinate. (d) Same as in (b) plotted in logarithmic time coordinate.

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