Image Details

Choose export citation format:

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 11.

Difference between the power-law exponents α from the calculation without time delays to that with time delays as a function of (horizontal axis) and thetav (vertical axis). The cases in the upper-right-hand corner of the plot are heavily obscured. The black contour curves there represent, respectively, from bottom to top .

Other Images in This Article
Copyright and Terms & Conditions