Fig. A.8

Dependence of the Brγ line profile on screening caused by an optically thick, dusty disk wind. The solid line represents the unscreened line profile of model 2 (see Table A.1) with f = 5, while the long-dashed (Hd = 100 R∗; θ = 20°) and dot-dashed (Hd = 130 R∗, θ = 25°) lines show models with screening. For all models shown, the inclination angle is i = 70°. See text for further details.
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