Free Access

Fig. 8

thumbnail

Time evolution for the M1 model of H- and He-burning luminosities (upper panel) and mass coordinate of the H-shell, of the inner border of the convective envelope, of the mass extension of the flash-driven convective shell, and of the convective core during central He-burning (lower panel). We set t = 0 at the end of the accretion phase.

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.