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Fig. 16.
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Stellar metallicity distribution of the simulation without any early feedback mechanism (black curve, 0.02 Z⊙/noESF) in comparison with 0.02 Z⊙/noRT and 0.02 Z⊙/full. Stars with extremely high metallicity (log(Z/Z⊙) > 1) can be formed from the unmixed ejecta in 0.02 Z⊙/noESF due to the absence of early feedback.
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