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Fig. 5.

image

Comparison of average radial profiles of the projected models of segregated (blue) and non-segregated clusters (red) with the real ONC (black). Only the models with pre-main sequence eigenevolution are plotted. Three time frames are shown, and two mass groups are compared in each model (m ≥ 5 M with a solid line and m <  5 M with a dashed line). The p-values for these groups are plotted in Fig. 6. All three models are modified by artificial extinction and scaling of the low-mass stars along the y-axis, as discussed in Paper I.

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