Open Access

Fig. B.3

image

SAD configurations, settled from rin = 1 with αv= 0.1, fed with an increasing infrom left to right: 0.01, 1, 100. Top panels: disk effective temperature Teff (solid lines) and ratio qadvqturb (dashed lines). Bottom panels: associated disk spectra. The dashed lines are the spectra emitted from each disk annulus whereas the solid black lines are the total integrated spectrum. A red color (in dots and spectra) describes annuli dominated by advection, whereas a green color (triangles and spectra) describes a negative advection term (see text).

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