Fig. 12
Dependence on stellar metallicity of the final surface overabundance distributions [X/Fe] of the 28 s-only nuclei at the surface of a 2 M⊙ model resulting from the LM scheme with Dmin = 103 cm2/ s, p = 1 and the DM formulation with Dmin = 109 cm2/ s, p = 5. In both cases, fover = 0.1 is taken. Four metallicities [Fe/H] = 0, −0.5, −1 and −2 have been considered.
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