Fig. 13
Initial vs. final mass relation plotted for several models: Padova tracks (two sets at solar and one at subsolar metallicity); Weidemann (2000); Weiss & Ferguson (2009) (solar metallicity). The open circles follow the IFMR interpolated from Blöcker (1995). The solid line follows IFMR as defined by Eq. (12); the filled dots correspond to the best-fit IFMR described in the text.
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