Fig. 5
Download original image
X-ray luminosity generated by wind accretion as a function of X-ray irradiation after Eq. (11) accounting for the dependence of the terminal velocity and the mass flux on X-ray irradiation via Eqs. (8) and (9). The figure was plotted for individual model stars from Table 1 and for different binary separations labeled in the plots. The pink line denotes the one-to-one relation.
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.