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GRMHD Prediction of Coronal Variability in Accreting Black Holes

  • Authors: Scott C. Noble and Julian H. Krolik

NOBLE & KROLIK 2009 The Astrophysical Journal 703 964.

  • Provider: AAS Journals

Caption: Figure 5.

Exponents α of the best power-law fits to the power spectra of the light curves as functions of (horizontal axis) and inclination angle (vertical axis). The departures from α ≈ −2 in the upper-right-hand corner of the plot are caused by the disk's self-obscuration. The black curves represent contours of R o . From bottom to top, .

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