\begin{table}%t15
%\centering
\par
\caption{Sample stars with Li upper limits. The stars with a $*$ lie in the 
ranges in effective temperature and metallicity chosen to delimitate the Li plateau.
The others are either cooler or more metal-rich. The~$\#$ indicates the stars
for which a {\it v}~sin{\it i} value higher than 4.5~km~s$^{-1}$ could
be derived by Ryan et~al. (\cite{Ryan02}) or Ryan \& Elliott (\cite{Ryan04}). See the text for more 
details.\label{tab15}}
\footnotesize {
{
\begin{tabular}{cccccccc}
\noalign{\smallskip}
\hline
\hline
\noalign{\smallskip}
 HIP & &  & \teff & Log $L/L_{\odot}$ & [Fe/H] & Li u.l. & single   \\
     & &  &       &                   &        &         & /binary  \\
\noalign{\smallskip}
\hline
Dwarfs \\
\hline
72561 &$^*$&$\#$&  6388 & $-0.12\pm0.30$  & --1.66  & 1.639 & b \\
100682 &$^*$&$\#$&  6362 & $-0.12\pm0.20$  & --2.83  & 1.088 & b \\
67655   & &      &  5429 & $-0.38\pm0.04$  & --1.03  & 1.245 & s \\
67863    & &     &  5683 & $-0.04\pm0.04$  & --0.88  & 1.338 & s \\
\hline
Subgiants \\
\hline
81276 &$^*$&$\#$&  6523 &  $0.76\pm0.58$  & --1.50  & 1.705 & b \\
83320 &$^*$&$\#$&  5984 &  $0.71\pm0.77$  & --2.56  & 1.265 & s \\
55022  & &$\#$&  6367 &  $0.50\pm0.14$  & --1.29  & 1.313 & s \\
60719   & &      &  5319 &  $1.44\pm0.21$  & --2.32  & 0.789 & s \\
\hline
\end{tabular}
}
}
\end{table}