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Fig. A.1.
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Abundance profiles of the SERIES I hybrid stellar model with 1.8 M⊙, Z = 0.02; fOV = 0.014. The left panel refers to the structure when log(ρc/g cm−3)≃9.0 (indicated by the black cross-mark in Fig. 3). The right panel shows the final chemical composition of the model.
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