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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. 7.

Skewness function as computed for two model light curves generated using eq. (6) with g(t) parameters equal to those of Fig. 6 and two different values of f, (a) ﹩f=2﹩ and (b) ﹩f=10﹩. The change in the sign of skewness with f at short timescales is apparent in the figure.
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