Fig. 9.
Mass functions for annuli of 0–3.1 pc, 3.1–9 pc, 9–18 pc, and 18–30 pc from the cluster centre scaled to a volume of one cubic parsec and mass bins of 0.1 dex in logarithmic units assuming an age of 650 Myr. Overplotted with a thick red line is the lognormal form of the field mass function (Chabrier 2003) normalised to one and multiplied by the most populated bin in the volume considered.
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