Fig. 8
Slim, optically thick JED configuration with ṁin = 2 at rin = 1 and (μ = 0.1, ξ = 0.1, ms = 1.5, b = 0.3). Left: Effective temperature as a function of the radius. Right: Spectrum emitted at each disk radius r (dashed lines, same color code as in the left panel). The solid lines are the overall disk spectra, i.e., the sum of the contributions from each disk annulus down to the inner radius rin. The inset shows the corresponding photon index Γ and high-energy cutoff Ecut, obtained with a fit E2−Γe−(E∕Ecut).
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