Fig. 9.

Single BH mass distribution in the three Galactic components for model B. In model B we assumed that the CE phase with an HG star donor always leads to a binary system merger. The mass of the objects thata formed in merger is estimated as a lower limit assuming total mass loss from the second merging object (except for two CO mergers).
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.