Interactions among binary black holes in star clusters: Eccentric gravitational wave captures and triple formation

Open Access

Fig. 6

Correction factor f(α) (defined in Sect. 4.1) as a function of the semimajor axes ratio α. A value of $f (α) > 1$ $f(\alpha)>1$ implies that the binarybinary interaction is more likely to trigger a GW merger than a binarysingle interaction where the binary has semimajor axis a_min.

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.