Table 2: Abundances obtained from least-square fittings for normal stars with metallicities corresponding to our sample of barium stars. Each set of five lines corresponds to the normal star with the same metallicity as the barium star indicated in parenthesis. $\log\epsilon(X)$ corresponds to $\log\epsilon_{\rm nor}(X)$ and $\epsilon \sb {\rm s,r,p}(X)$ corresponds to $\epsilon _{\rm s,r,p} (X)_{\rm nor}$ from Eq. (2). $\epsilon _{\rm o}(X)$ is from Eq. (6). The full table is only available in electronic form at the CDS.
  Sr Y Zr Mo Ba La Ce ...
    [Fe/H] = -0.06 (HD 749)    
$\log\epsilon(X)$ $2.85\pm0.18$ $2.17\pm0.20$ $2.57\pm0.17$ $1.84\pm0.37$ $2.04\pm0.18$ $1.31\pm0.22$ $1.44\pm0.19$ ...
$\epsilon\sb {\rm s}(X)$ $594.4\pm51.0$ $136.8\pm63.2$ $307.4\pm20.1$ $34.1\pm29.2$ $87.7\pm36.1$ $12.5\pm6.3$ $20.9\pm9.0$ ...
$\epsilon\sb {\rm r}(X)$ $0.00\pm0.00$ $11.9\pm5.5$ $58.9\pm23.0$ $17.9\pm15.4$ $20.6\pm8.5$ $7.7\pm3.8$ $6.5\pm2.8$ ...
$\epsilon\sb {\rm p}(X)$ $109.0\pm46.0$ $0.0\pm0.0$ $4.1\pm1.6$ $16.7\pm14.3$ $0.2\pm0.1$ $0.0\pm0.0$ $0.1\pm0.0$ ...
$\epsilon\sb {\rm o}(X)$ $109.0\pm46.0$ $11.9\pm5.5$ $63.0\pm24.6$ $34.6\pm29.7$ $20.8\pm8.6$ $7.7\pm3.8$ $6.6\pm2.8$ ...
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