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Fig. 6


Field-star decontaminated CMDs (light-shaded circles) of Collinder 197 (left) and Pismis 5 (right) compared to a single realisation taken from the respective simulations (empty circles). The extraction radii are 10′ (Collinder 197) and 6′ (Pismis 5). Isochrones representing the star-formation history have been set according to the mean parameters (Table 2). Insets show the DR distribution.

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