Fig. 9
Geometry of the magnetosphere model assumed in this paper. The matter accretes onto the star within thin cones (gray) with the inner and outer half opening angles θin and θout. The outer parts of the magnetospheric accreting regions are assumed to be negligible as contributors to the line emission because of their lower gas temperature.
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.