Fig. 3
Sketch of the scheme for radiative transfer calculations. Stellar light moves outwards from the star to a point at which some of the light is scattered towards a distant observer. From this point light travels through the outer (case A) or first through the inner and then the outer (case B) before it reaches the boundary of our model.
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.