Free Access

Fig. 18

thumbnail

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).

This figure is made of several images, please see below:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.