Fig. 6

Optical depth at infinity for 1 GeV photons interacting with non-thermal hard X-rays (10−100 keV). Gamma rays are injected on the axis of the accretion disk at an altitude z (r ≡ 0) and with an inclination ψ = 30°. The corona X-ray density is homogeneous and isotropic in a spherical region of radius Rc = 6 rg (solid line), 60 rg (dashed line) and 600 rg (dotted-dashed line) around the compact object, here a 20 M⊙ black hole (6 rg = 1.8 × 107 cm). Outside, the X-ray flux is radial. The total power injected in hard X-rays is Lc = 5 × 1036 erg s-1. The gamma-ray optical depth from the disk only is shown with the red dashed line for comparison.
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