Fig. 13.


Each pair of panels (from top to bottom) shows the cluster and its tidal tails in X − Y Galactic coordinates rotated so that the VY component is horizontal. This allows us to plot the histogram along the tail and to reduce projection effects caused by the spatial alignment of the tail. Upper two double panels: models M1 and M5 at the age of 655 Myr. Lower two double panels: data selected based on the M1 and M5 models.

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