Free Access

Fig. 6


Relative velocity of the flying-by cluster members versus the tidal radius with respect to the flying-by cluster members in units of the half-mass radius of the model galaxy at the moment of closest approach. The colour scale denotes the approximate energy that the flying-by cluster members inject into the stellar component of the galaxy, in units of the total energy of the stellar component.

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.