Free Access
Fig. 2
Cartoon illustrating the possible occurrence of ECSN after the formation of a He star in the scenarios involved for the formation of high- (left) and low- (right) mass X-ray binaries. This cartoon has been adapted from Tauris & van den Heuvel (2006). The numbers indicate the masses of the stellar components.
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.