Fig. 1
Comparison of model clusters with 10 000 stars and a half-mass radius of 1 pc obeying a Plummer distribution (open circles) with those of a King (W0 = 12) distribution. Here a) shows the number of stars as a function of the radial distance to the cluster centre, whereas b) shows the number of stars of a given surface density and c) the same in cumulative normalized form.
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