Open Access

Fig. 12.

image

Download original image

Normalized distribution of cos(Ψstar, BH) for secondary BHs at z = 0.18. The sample consists of 30 BHs with a mass greater than 2 × 104M. Contrary to primary BHs, the distribution tends to be uniform suggesting no privileged orientation between the BH spin and the angular momentum of their host galaxies.

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.