\begin{table}%t1
%\centering
\par
\caption{\label{tab:modelinfo}Summary of the best fitting solar-abundance and metal-poor adiabatic and nonadiabatic models for the frequencies given by A: \cite{gru08} and B: \cite{apo08}. 
}
\small\begin{tabular}{lcc cccccc cc}
\hline
\hline \noalign{\smallskip}
Source & ($Y$, $Z$)&adia./nonadia.&$M$ & $R$ & $T_{\rm eff}$ & $L$ & log~$g$ & Age & $\chi^2$ &  $Q$\\
            &          &                       &[$M_{\sun}$] & [$R_{\sun}$]             &[$K$]     &  [$L_{\sun}$]            &[cm~${\rm s}^{-2}$]&[Gyr]&&\\
\hline
A&(0.27, 0.02) &nonadiabatic& {\bf 1.325} & {\bf 1.49} & {\bf 6484} & {\bf 3.52} & {\bf 4.22} & {\bf 2.15}  & {\bf 0.79} & {\bf 0.090}\\
A &         --        &      adiabatic&        1.325  &       1.49  &        6485  &       3.52  &        4.21  &        2.13   &       1.0  &                0.081 \\
\par
A &(0.24, 0.008)&nonadiabatic& 1.205 & 1.43 & 6644 & 3.57 & 4.22 & 2.98 &  2.26 &  0.043 \\
A &         --         &      adiabatic& 1.205 & 1.43 & 6641 & 3.57 & 4.21 & 2.99 &  4.16 &  0.017 \\
\hline
B&(0.27, 0.02) &nonadiabatic& 1.325 & 1.49 & 6487 & 3.52 & 4.22& 2.14&  19.6 &  $1.8\times 10^{-5}$\\
\par
 B$^{*}$&      --    &nonadiabatic& 1.600 & 1.53 & 7447 & 6.42 & 4.28 &0.18 &  44.9 & $8.3\times 10^{-11}$\\
 B&(0.24, 0.008)&nonadiabatic& 1.205 & 1.43 & 6645 & 3.57 & 4.22 &2.97 &  27.5 & $3.7\times 10^{-7}$\\
\hline
& &&& $1.46\pm0.05$ & $6500\pm 75$   &$3.58\pm 0.1$& $4.0\pm0.15$&&&\\
\hline
\end{tabular}\vspace*{5mm}
\end{table}