Free Access

Fig. 7.

image

Schematic representation of the model scenario. The photo-ionisation wake is responsible for the increased absorption column asymmetry before the eclipse. An accretion wake might also be present and increase absorption in phases previous to that of the eclipse. This figure is adapted from Kaper et al. (1994).

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.