Fig. 9.
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Distribution of PMS stars (panel a) and massive stars (panel b) in the field. The younger PMS stars are indicated in blue and the older ones in orange. The younger massive stars are indicated in blue and the older ones in red. In panel b), two circles are drawn: one indicating a 25″ radius centred on the cluster, and one indicating the 15″ region used to estimate the background contribution to the stellar density profile.
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