Free Access

Fig. A.2


Stellar mass for the dwarf only experiencing tidal forces in the standard GEAR implementation (blue) and in the rotating reference with the Mid-v scheme (green dash) and with the It-v scheme (red dash-dot) and the It-v scheme with a low step size (green dotted). The beginning of the orbit is shown with a vertical dotted line. For the first ~1.5 Gyr, the stellar mass is basically the same with similar bursts (see Fig. A.3), beyond this, however, the Mid-v scheme flattens out, still producing stars for another ~1.5 Gyr, but at a lower rate. The drop in stellar mass at the end in the rotation schemes is due to stellar particles being deleted as they cross the boundaries. This drop is lower in the low step size due to better simulation of the dwarf core (see Fig. A.4).

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.