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Full radiative coupling in two-phase models for accreting black holes

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Academic year: 2021

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Figure

Fig. 1. The infinite slab accretion disc corona and spherical cloud ge- ge-ometry. The hot slab is divided into 10 horizontal layers with  homo-geneous temperatures
Fig. 2. Angle averaged escaping spectra for covering fractions C = 0.3 (left-hand side) and C = 0.5 (right-hand side)
Fig. 3. X-ray albedo (i.e. fraction of the reflected /reprocessed luminosity emitted above 1 keV) as a function of the ionization parameter ξ (left) and spectral index, Γ p (right), of the simulated spectra obtained from fits with the PEXRAV model (see tex
Fig. 4. Reflection amplitude R and spectral index Γ p of the simulated spectra obtained from fits with the PEXRAV model (see text and Table 1).
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