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

Open Access

Fig. 3.

Central abundances of ¹²C (upper left), ¹⁶O (lower left), ²³Na (upper right), and ²⁷Al (lower right) relative to their initial abundance for each Z as a function of core He abundance during the MS evolution of 100 M_⊙ models.

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