Table 6: Contributions of s- and r-processes for the abundances of Hf, Ru, Y, Eu, Sm, and Nd in solar system, following Arlandini et al. (1999). The last column is the sum of s- and r-processes.
\begin{displaymath}\begin{tabular}{rccc} \hline\hline \noalign{\smallskip } El. ... ... & 36.84 & 92.3 \\ \noalign{\smallskip } \hline \end{tabular} \end{displaymath}


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