Fig. 2.
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Surface abundances ([X/H] = log(X/H) − log(X/H)⊙) with respect to the hydrogen surface abundance as a function of fraction of initial hydrogen burnt in the convective core. The surface abundances are scaled with the Solar composition as determined by Magg et al. (2022). Solid lines correspond to ζ = 0, dashed lines to ζ = −0.5, and dotted lines to ζ = −1.
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