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Fig. 10.
Emergent spectra (top panel) and temperature structures (bottom panel) of the models with different accretion luminosities (ℓa = 0.01, 0.03, 0.05, 0.1, 0.3, and 0.5). The fit to the spectrum above 15 keV with an exponential cutoff power law with Γ = 2.25, Ecut = 42 keV is shown for ℓa = 0.5.
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