The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity

Open Access

Fig. 17.

Diluted ejected from initially 40% critically rotating 80–300 M_⊙ models calculated at 1/30th Z_⊙. Observations of stars in NGC 5904 are shown as in Fig. 11, adopted from Carretta et al. (2009). Dilution factors ranging from 1 to 100 are shown for each model (assorted symbols) and connected for each f value (coloured lines).

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