Fig. 6
Overabundance distributions [X/Fe] for the 28 s-only nuclei inside a region of 0.01 M⊙ around Mr = 0.595−0.605M⊙ at the end of the 8th interpulse of our 2 M⊙[Fe/H] = −0.5 model star. The results are shown for different LM conditions, i.e. different values of p (upper panel) or Dmin (in cm2/s; lower panel); in all cases, fover = 0.1 is assumed.
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