Table 1: Values of the "indicators'' of the s-process efficiency (see text) for stellar models with mixing length parameter $\alpha =1.7$. The overshooting parameter value used in the stellar evolution code isreported in the first column.
f F0 $\tilde{F_0}$ $A_{\max}$ $n_{\rm c}$ m.c.z.m.e. Duration [s]
10-5 99.88 6.57 91-96 4.24 $5.31~M_{\odot}$ $2.43\times10^{13}$
0.01 246.13 11.16 94-104 5.22 $6.39~M_{\odot}$ $2.27\times10^{13}$
0.015 216.74 10.13 94-104 5.09 $6.87~M_{\odot}$ $2.09\times10^{13}$
0.02 257.81 11.57 94-104 5.32 $7.23~M_{\odot}$ $2.06\times10^{13}$
0.025 236.40 10.82 94-104 5.20 $7.31~M_{\odot}$ $2.16\times10^{13}$
0.03 304.17 13.20 96-104 5.55 $7.97~M_{\odot}$ $2.48\times10^{13}$
0.035 310.39 13.49 96-104 5.58 $8.67~M_{\odot}$ $2.44\times10^{13}$


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