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Fig. 11
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Comparison of the Larson (1982), Larson (2003), and Kroupa-Weidner (Weidner & Kroupa 2004, 2006) maximum stellar masses as in Weidner & Kroupa (2006) Fig. 1 but recalculated for the range in stellar masses used here (0.08-100 M⊙) and a Chabrier IMF. The dashed line at 100 M⊙ gives the “stochastic” mass limit.
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