Fig. 12
Comparison of the Brγ line profiles (normalized to the star continuum) for the disk wind model DW3 (blue) and magnetospheric accretion model MS6 (red) for a Herbig Ae star. The total line profile (the combination of the disk wind and magnetospheric accretion model profiles) is shown as a black line. The profiles for 20° and 60° inclination angles are presented.
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