\begin{table}%t4 %\centering \par \caption{\label{solar}Mass fractions of several elements yielded by the Fran\c{c}ois et~al. (\cite{Francois2004}) model and the delay model at the galactic age of 9.5 Gyr compared to the solar values of Asplund et~al. (\cite{Asplund2005}).} \small \begin{tabular}{c|c|ccccc} \hline\hline & $X_{\odot {\rm oss}} $ &\multicolumn{5}{c}{ $X_{\odot {\rm th}} $}\\ \hline %\noalign{\smallskip} & Asplund et~al. (\cite{Asplund2005}) &Fran\c{c}ois et~al. (\cite{Francois2004}) &0.1 Gyr &0.2 Gyr &0.5 Gyr &1 Gyr \\ \hline He & $2.55 \times 10^{-1}$ & $2.52 \times 10^{-1}$& $2.52 \times 10^{-1}$ & $2.52 \times 10^{-1}$ &$2.52 \times 10^{-1}$ &$2.52 \times 10^{-1}$ \\ % & & & & & &\\ C & $2.21 \times 10^{-3}$ & $2.03 \times 10^{-3}$&$2.05 \times 10^{-3}$ &$2.06 \times 10^{-3}$ &$2.11 \times 10^{-3}$ & $2.17 \times 10^{-3}$ \\ % & & & & & &\\ N & $6.32 \times 10^{-4}$ & $9.73 \times 10^{-4}$ &$9.75 \times 10^{-4}$ &$9.77 \times 10^{-4}$ &$9.81 \times 10^{-4}$ &$9.85 \times 10^{-4}$\\ % & & & & & & \\ O & $5.48 \times 10^{-3}$ & $5.27 \times 10^{-3}$ & $5.31 \times 10^{-3}$ & $5.35 \times 10^{-3}$ & $5.46 \times 10^{-3}$ & $5.62 \times 10^{-3}$ \\ % & & & & & &\\ \par Mg & $6.17 \times 10^{-4}$ &$6.66 \times 10^{-4}$ &$6.70 \times 10^{-4}$ &$6.74 \times 10^{-4}$ & $6.86 \times 10^{-4}$& $7.03 \times 10^{-4}$\\ % & & & & & &\\ \par Si & $6.80\times 10^{-4}$ &$8.14 \times 10^{-4}$ &$8.17 \times 10^{-4}$ &$8.20 \times 10^{-4}$ &$8.30 \times 10^{-4}$ &$8.43 \times 10^{-4}$ \\ % & & & & & &\\ S & $3.31 \times 10^{-4}$ & $3.95\times 10^{-4}$ & $3.97\times 10^{-4}$ & $3.98\times 10^{-4}$ &$4.03\times 10^{-4}$ &$4.09\times 10^{-4}$\\ % & & & & & &\\ Ca & $6.13 \times 10^{-5}$ & $5.40 \times 10^{-5}$ &$5.42 \times 10^{-5}$ &$5.44 \times 10^{-5}$ &$5.50 \times 10^{-5}$ &$5.58 \times 10^{-5}$ \\ % & & & & & &\\ Fe & $ 1.18 \times 10^{-3}$ & $1.14 \times 10^{-3}$ & $1.15 \times 10^{-3}$ &$1.15 \times 10^{-3}$ &$1.15 \times 10^{-3}$ &$1.16 \times 10^{-3}$\\ % & & & & & &\\ \hline \end{tabular} \end{table}