\begin{table}%T2
\par
\caption{\label{tab2}Li abundance in a volume-limited sample of stars without detected giant
planets from Santos et~al.\ (\cite{Santos2001}).}
%\centering
\par
\begin{tabular}{lcccrc}
\hline\hline
\noalign{\smallskip}
Star & $T_{\rm eff}$ & $\log{g}$  & $\xi_t$  & [Fe/H]  & $\log \epsilon({\rm Li}$) \\
     & (K)  &  (cm~s$^{-2}$) & (km~s$^{-1}$) &  &    \\
\noalign{\smallskip}\hline  \noalign{\smallskip}
\object{HD~1581 }  & 5940 & 4.44 & 1.13 & $-$0.15 & 2.35     \\
\object{HD~4391 }  & 5955 & 4.85 & 1.22 & 0.01    & $<$1.16  \\
\object{HD~5133 }  & 5015 & 4.82 & 0.92 & $-$0.08 & $<$0.01  \\
\object{HD~7570 }  & 6135 & 4.42 & 1.46 & 0.17    & 2.91     \\
\object{HD~10360}  & 5045 & 4.77 & 0.89 & $-$0.19 & $<$0.05  \\
\object{HD~10647}  & 6130 & 4.45 & 1.31 & $-$0.03 & 2.80     \\
\object{HD~10700}  & 5370 & 4.70 & 1.01 & $-$0.50 & $<$0.43  \\
\object{HD~14412}  & 5410 & 4.70 & 1.01 & $-$0.44 & $<$0.47  \\
\object{HD~20010}  & 6240 & 4.27 & 2.23 & $-$0.20 & 2.10     \\
\object{HD~20766}  & 5770 & 4.68 & 1.24 & $-$0.20 & $<$1.00  \\
\object{HD~20794}  & 5465 & 4.62 & 1.04 & $-$0.36 & $<$0.53  \\
\object{HD~20807}  & 5865 & 4.59 & 1.28 & $-$0.22 & $<$1.09  \\
\object{HD~23356}  & 5035 & 4.73 & 0.96 & $-$0.05 & $<$0.34  \\
\object{HD~23484}  & 5230 & 4.62 & 1.13 & 0.10    & $<$0.44  \\
\object{HD~26965A} & 5185 & 4.73 & 0.75 & $-$0.26 & $<$0.22  \\
\object{HD~30495 } & 5880 & 4.67 & 1.29 & 0.03    & 2.45     \\
\object{HD~36435 } & 5510 & 4.78 & 1.15 & 0.03    & 1.69     \\
\object{HD~38858 } & 5750 & 4.56 & 1.22 & $-$0.22 & 1.64    \\
\object{HD~40307 } & 4925 & 4.57 & 0.79 &$-$0.25  & $<$$ -0.09$ \\
\object{HD~43162 } & 5630 & 4.57 & 1.36 &$-$0.02  & 2.33     \\
\object{HD~43834 } & 5620 & 4.56 & 1.10 & 0.12    & 2.32     \\
\object{HD~50281A} & 4790 & 4.75 & 0.85 & 0.07    & $<$$ -0.27$ \\
\object{HD~53705 } & 5810 & 4.40 & 1.18 & $-$0.19 & 1.04     \\
\object{HD~53706 } & 5315 & 4.50 & 0.90 & $-$0.22 & $<$0.24  \\
\object{HD~65907A} & 5940 & 4.56 & 1.19 & $-$0.29 & $<$0.98  \\
\object{HD~69830 } & 5455 & 4.56 & 0.98 & 0.00    & $<$0.51  \\
\object{HD~72673 } & 5290 & 4.68 & 0.81 & $-$0.33 & $<$0.52  \\
\object{HD~76151 } & 5825 & 4.62 & 1.08 & 0.15    & 1.90     \\
\object{HD~84117 } & 6140 & 4.35 & 1.38 & $-$0.04 & 2.62     \\
\object{HD~189567} & 5750 & 4.57 & 1.21 & $-$0.23 & $<$0.81  \\
\object{HD~191408A}& 5025 & 4.62 & 0.74 & $-$0.51 & $<$0.13  \\
\object{HD~192310 }& 5125 & 4.63 & 0.88 & 0.05    & $<$0.24  \\
\object{HD~196761 }& 5460 & 4.62 & 1.00 & $-$0.27 & $<$0.70  \\
\object{HD~207129 }& 5910 & 4.53 & 1.21 & $-$0.01 & 2.33     \\
\object{HD~209100 }& 4700 & 4.68 & 0.60 & 0.01    & $<$$-0.39$ \\
\object{HD~211415 }& 5925 & 4.65 & 1.27 & $-$0.16 & 1.95     \\
\object{HD~222237 }& 4770 & 4.79 & 0.35 & $-$0.22 & $< $$-0.26$ \\
\object{HD~222335 }& 5310 & 4.64 & 0.97 & $-$0.10 & $<$0.35  \\
\hline
\end{tabular}
\end{table}