Fig. C.1
Radial gravitational potential profiles of the four alternative host galaxy representation and for the N-body live host galaxy (black). The alternative models cover a variety of central and outer slopes allow testing of the influence of those on satellite tidal tails. The varying thickness of the profile lines reflects the nonspherical symmetry of the potentials.
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.