Fig. 8
Cluster mass function assuming an age of 30 Myr (Manzi et al. 2008) and a distance of 350 pc. The conversion from magnitudes into masses made use of the NextGen and DUSTY models (Baraffe et al. 1998; Chabrier et al. 2000). Values are given in Table 4. The vertical dot-dashed lines represent the GCS completeness limits in IC 4665.
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