Open Access
Fig. 1
Download original image
Fraction ffrom of BCOs with WR–CO progenitors for all the metallicities (columns), αCE efficiencies (rows), and combinations of CCSN and natal kick models tested in this work (horizontal entries, see Table 1). We distinguish BCOs into BBHs, BNSs and BHNSs; WR–CO progenitors into systems with a WR star and a BH or NS.
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.