Free Access
Fig. 12.
Prediction of our population synthesis model for the probability of OB stars to have a BH companion as a function of the observed orbital period (top) and of the observed radial velocity semi-amplitude (bottom), respectively.
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.