Stellar density profiles at 4t_ff (blue points) are compared with the analytically predicted Plummer profile for the stellar distribution (dashed orange line), as well as best-fit Plummer (dashed green) and EFF (dash-dotted magenta) models. The mass of the most massive star formed in each simulation is indicated in the lower left corner of each panel. The panel marked with a ★ (n3s3) is shown at a slightly earlier time; see also the text for details on subcluster cases.