Fig. B.1.
Average positions of the most massive stars that are in the top 10 % of the total mass of the cluster (solid lines). Models with 1.2k, 2.4k, 4.7k, and 9.2k stars are plotted from top to bottom. The data are averaged over all realisations of a given model. For reference, we also plot the half-mass radius with a dashed line. Time extends to ≈18 Myr.
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