Fig. 10
Tangential velocity profiles of the post-merger stellar disk as function of height from the galaxy mid-plane in dissipationless (upper panels) and dissipational (lower panels) minor mergers with a gas mass fraction of 0.2. Profiles are shown at different disk scale lengths, rd, from the galaxy center along the major axis of the galactic mid-plane.
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.