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Fig. 18


Brγ line profile (model A1) normalized to the continuum of the accretion disk plus continuum of the star with absorption of the disk and star continuum radiation by the opaque disk wind taken into account. Top: i = 50°, middle: i = 70° and bottom: i = 80°. The ratio of the disk continuum to the star continuum is R1a); R2b); R3c); and R4d) (from Table 3).

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