Fig. 9
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Stellar mass spectrum of the two models at SFE=0.05 (dotted lines) and SFE=0.1 (plain lines). Outflows do not affect the number of low-mass stars (i.e., below a few 0.1 M⊙) but affect the number of more massive stars. In particular, they tend to increase the number of stars with masses around 0.3 M⊙ and reduce the number of the most massive stars.
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