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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