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Fig. C.1.

image

a1, a2: dependence on the accretion rate, = 0.01 (red, dotted), 0.1 (green, dashed), and 1.0 (blue, solid). (a1) log Tp as a function of log r and (a2) log νLν with log ν. (b1, b2) Dependence on mass of BH, MBH = 102 (blue, solid), 104 (green, dashed), 106 (red, dotted) in the production of γ rays. (b1) log Tp as a function of log r and in (b2) the corresponding spectra are plotted. The gamma ray emission is presented in grey.

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