Fig. 4
Differential and cumulative local surface-density distribution for stars from two Plummer-shaped (a) and b)) and two King-shaped c) model clusters. The approximate mean densities of each individual cluster is 10 stars pc-3 and 1000 stars pc-3 in a) and 100 stars pc-3, and 1000 stars pc-3 in b) and c). For each cluster mode, 10 000 stars were considered.
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