Free Access

Fig. 5

image

Position of simulated stars belonging to pop. A (red crosses) and pop. B (black open circles), projected in the plane of the sky (the xz plane of the simulation), at three different times (t = 2.5, 4.8 and 6.9 Myr since the beginning of the simulation) in run 1. The centre of the frame is the centre of mass of the entire cluster (pop. A + pop. B). We note that pop. B expands much faster than pop. A given its supervirial condition. Stars belonging to pop. B can be found at >10 pc from the centre of pop. A.

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.