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Fig. 17


Influence of screening by an optically thick, dusty disk wind or a flared dusty disk (scenario in Fig. 15 right) on the Brγ line profile (model B6; inclination angle i = 70°; see Table 1). The solid line represents the unscreened line profile, while the long-dashed (hs = 100  R; θ = 20°), short-dashed (hs = 120  R; θ = 20°), and dotted-dashed (hs = 130  R; θ = 25°) lines show models with screening.

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