Fig. B.2.
Evolution of a cluster with N = 1000 stars, total mass Mstars = 104 M⊙ and Rv = 1.0 pc in a background potential with mass Mext = 103 M⊙. Top panel: fraction of stars that were ejected from the cluster. Bottom panel: Lagrangian radius and the vertical green line marks the moment of core collapse. The time is presented in units of the crossing time of the cluster.
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