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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 10.

Left: normalized light curves obtained from the calculation ignoring time delay effects (dotted curve) and taking them into account (solid curve). Right: normalized power spectra of these light curves compared to their best power-law fits; the dashed line represents the best fit to the data with time delay effects, the dash-dot to the data in which time delays were ignored. Both light curves are for thetav = 29° and .

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