Fig. 6.
Transformed mass-loss rate versus Fe mass fraction for WC4 and WC5 stars at different metallicities: The extragalactic results are taken from Crowther et al. (2002, LMC) and Abbott et al. (2003; M 33 outskirts). The solid line gives the linear regression fit to the data points. The Galactic WC4 and WC5 plot symbols have a slight shift compared to the actual datapoint to ensure visibility.
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