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Fig. 10
Surface overabundance distributions [X/Fe] for the 28 s-only nuclei at the end of the AGB phase of a 2 M⊙[Fe/H] = −0.5 model star computed with the DM overshoot formalism and 9 different sets of mixing parameters, i.e. Dmin = 103,106, and 109 cm2/ s, p = 1/5,1,5 and fover = 0.1.
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