Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase

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Fig. 3

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As in Fig. 1, but for Z = 0.02, M = 25 M_⊙ stellar models with overshooting parameter f = 10^-5 and 0.01 (see labels). Solid lines shown our results obtained with stellar models using the NACRE rate for ; while dashed lines are data from Paper I and Paper II, using an older rate.

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