\documentstyle{l-aa}
\begin{document}
\setcounter{table}{+1}
\begin{table*}
\caption{Li abundances for sample stars}
\begin{tabular}{lcrcccc} \hline
 & & & & & &\\
\multispan{4}{IC~2602\hfill}\\
 & & & & & &\\
star & Teff & $\Delta$Teff & EW(Li) & $\log$ n(Li)$_{\rm LTE}$& $\log$ n(Li)$_{\rm NLTE}$ &$\Delta \log$ n(Li) \\
      & (K)   & (K) & (m\AA) &    &     &    \\
 & & & & & & \\
W79  & 5260 & 57      & 142 $\pm$ 5 & 2.3 &    2.4      & 0.14 \\
R1   & 5050 & 89      & 204 $\pm$ 7 & 2.4 &    2.4      & 0.18 \\
R8A  & 5930 & 86      & 178 $\pm$ 9 & 3.2 &    3.1      & 0.20 \\
R15  & 4820 & 76      & 255 $\pm$15 & 2.4 &    2.4      & 0.24\\
R24A & 3780 & 100$^*$ & 112 $\pm$ 8 & 0.3 &    0.3      & 0.2$^*$ \\
R26  & 3540 & 100$^*$ & $\leq$ 100  & --- &  ---         & --- \\
R27  & 3830 & 100$^*$ & $\leq$ 50   & --- &  ---         & --- \\
R30  & 3440 & 100$^*$ & $\leq$ 80   & --- &  ---         & --- \\
R31  & 3480 & 100$^*$ & $\leq$ 55   & --- &  ---         & --- \\
R32  & 3540 & 100$^*$ & $\leq$ 60   & --- &  ---         & --- \\
R38  & 3330 & 100$^*$ & $\leq$ 50   & --- &  ---         & --- \\
R39  & 3310 & 100$^*$ & $\leq$ 80   & --- &  ---         & --- \\
R44  & 3630 & 100$^*$ & $\leq$ 70   & --- &  ---         & --- \\
R50  & 3590 & 100$^*$ & $\leq$ 50   & --- &  ---         & --- \\
R52  & 4580 & 53      & 262 $\pm$11 & 2.1 &     2.2      & 0.18 \\
R53B & 3340 & 100$^*$ & ---         & --- &  ---       & ---\\
R54A & 4260 & 93      & 189 $\pm$10 & 1.2 &  ---       & 0.21 \\
R57  & 3360 & 100$^*$ & $\leq$ 100  & --- &  ---         & --- \\
R66  & 5560 & 174     & 173 $\pm$10 & 2.8 &     2.8      & 0.3 \\
R67  & 3540 & 100$^*$ &  72 $\pm$12 & $-$0.3 &  ---      & 0.24$^*$ \\
R70  & 5760 & 62      & 172 $\pm$12 & 3.0 &     2.9      & 0.2 \\
R73A & 3340 & 100$^*$ & $\leq$ 60   & --- &  ---         & --- \\
R77  & 3910 & 100$^*$ & $\leq$ 30   & --- &  ---         & ---\\
R82  & 3330 & 100$^*$ & $\leq$ 56   & --- &  ---         & ---\\
R93  & 3980 & 10      &  60 $\pm$10 & 0.0 &  ---        & 0.12 \\
R96  & 4160 & 10      & 320 $\pm$12 & 2.0 &  ---         & 0.14  \\
& & &  & & & \\ \hline
& & &  & & & \\
\multispan{7}{Asterisks indicate stars for which errors in Teff could
not be directly estimated\hfill}\\
\end{tabular}
\end{table*}
%
\begin{table*}
\begin{tabular}{lrccccc} \\ \hline
 & & & & & & \\
\multispan{4}{IC~2391\hfill}\\
 & & & & & & \\
star & Teff & $\Delta$Teff & EW(Li) & $\log$ n(Li)$_{\rm LTE}$ & 
$\log$ n(Li)$_{\rm NLTE}$ &$\Delta \log$ n(Li) \\
      & (K) & (K)  & (m\AA) &  & &      \\
 & & & & & & \\
 VXR3A  & 5590 & 100$^*$ & 175$\pm$ 16 & 2.9 & 2.8 & 0.27$^*$\\
 VXR6A  & 3690 & 34      & $\leq$ 60   & --- &  --- &---\\
 VXR7   & 6470 & 100$^*$ & 116$\pm$  9 & 3.3 & 3.2 & 0.21$^*$\\
 VXR14  & 5780 & 106     & 162$\pm$ 11     & 3.0 & 2.9 & 0.23 \\
 VXR16A & 4970 & 73      & 302$\pm$ 12 & 3.0 & 2.8 & 0.21 \\
 VXR18A & 3990 & 25      &  55$\pm$ 15 & 0.0 &  --- & 0.18  \\
 VXR30  & 6470 & 100$^*$ & 109$\pm$ 12 & 3.3 & 3.2 & 0.24$^*$ \\
 VXR31  & 5630 & 100     & 182$\pm$ 10 & 3.0 & 2.9 & 0.22\\
 VXR44  & 6650 & 100$^*$ &  71$\pm$ 12 & 3.0 & 2.9 & 0.24$^*$ \\
 VXR49B & 3730 & 33      & $\leq$ 50   & --- & --- & --- \\
 VXR50A & 5050 & 76      & 239$\pm$ 13 & 2.6 & 2.6 & 0.22 \\
 VXR62A & 4841 & 67      & 250$\pm$ 15 & 2.4 & 2.4 & 0.23\\
 VXR65  & 3820 & 30      & $\leq$ 45   & --- & --- & --- \\
 VXR67A & 4750 & 63      & 255$\pm$ 16 & 2.3 & 2.3 & 0.27 \\
 VXR69A & 5080 & 77      & 251$\pm$ 17 & 2.7 & 2.7 & 0.25 \\
 VXR70  & 5557 & 97      & 182$\pm$ 10 & 2.9 & 2.8 & 0.22 \\
 VXR71A & 3360 & 15      & $\leq$ 70   & --- & --- & --- \\
 VXR72  & 5257 & 85      & 225$\pm$ 13 & 2.8 & 2.7 & 0.22\\
 VXR76A & 4343 & 43      & 204$\pm$ 11 & 1.4 & --- & 0.17 \\
 VXR77A & 6150 & 120     &  90$\pm$  8 & 2.9 & 2.8 & 0.22 \\
 VXR78  & 5630 & 100     & 178$\pm$ 10 & 2.9 & 2.8 & 0.22 \\
 VXR80A & 4720 & 61      & 232$\pm$ 34 & 2.3 & 2.2 & 0.37 \\
& & &  & & &\\ \hline
\end{tabular}
\end{table*}
\clearpage

\begin{table}
\caption{Li abundances for S89 sample}
\begin{tabular}{lcrcccc} \hline
 & & & & & &\\
star & Teff & $\Delta$Teff & EW(Li) & $\log$ n(Li)$_{\rm LTE}$ &
$\log$ n(Li)$_{\rm NLTE}$ &$\Delta \log$ n(Li) \\
      & (K) & (K)  & (m\AA) & &  &     \\
 & & & & & &\\
SHJM~1 & 5590 & 95  & 160  $\pm$ 10 & 2.8 & 2.7 & 0.22\\
SHJM~2 & 5970 & 147 & 140  $\pm$ 10 & 3.1 & 2.9 & 0.27\\
SHJM~3 & 4480 & 166 & 130  $\pm$  7 & 1.2 & --- & 0.77\\
SHJM~6 & 5050 & 75  & 190  $\pm$ 11 & 2.3 & 2.4 & 0.20\\
SHJM~7 & 4380 & 36  & $\leq$ 50  & $\leq$ 0.39& --- & ---  \\
SHJM~8 & 4020 & 98  & 90   $\pm$ 30 & 0.4 & --- & 0.38\\
SHJM~9 & 4030 & 87  & 100  $\pm$ 30 & 0.4 & --- & 0.37\\
SHJM~4 & 3558 & 20  & $\leq$ 50  & $\leq$ 0.& --- & ---  \\
SHJM~5 & 3893 & 28  & $\leq$ 200 & $\leq$ 1.1& --- & ---  \\
SHJM~10& 3580 & 20  & $\leq$ 100 & $\leq$ 0.46& --- & ---  \\
& &  &&  & &\\ \hline
\end{tabular}
\end{table}


\begin{table*}
\caption{Recomputed Li abundances for R97}
\begin{flushleft}
\begin{tabular}{rclcl}  \hline
  &   &     & & \\
star & Teff (R97)& \nli (R97) & Teff (new) & \nli (new) \\ 
     & (K) & & (K) & \\ 
  &   &   & & \\
R~ 3~~&5080& 2.74     & 5140 &2.79\\
R~ 7~~&6750& $>$ 2.97 & 6860 & 3.14\\
R~14~~&5080& 2.58     & 5150 & 2.65 \\
R~15~~&4900& 2.55     & 4820 & 2.44 \\
R~21~~&6430& 3.18     & 6320 & 3.10  \\
R~29~~&4440& 1.76     & 4440 & 1.77 \\
R~35~~&5770& 3.12     & 5820 & 3.12 \\
R~43~~&4840& 2.99     & 4740 & 2.89 \\
R~45~~&5810& 2.87     & 5800 & 2.87 \\
R~56~~&3910& $\leq$ 0.65& 3990 & 0.64 \\
R~58~~&5850& 3.26 (3.12) & 5780 &3.25 (3.06) \\
R~59~~&5240& 3.09     & 5060 & 2.91 \\
R~66~~&5730& 2.97     & 5560 & 2.83 \\
R~68~~&5110& 2.77     & 4880 & 2.57 \\
R~70~~&5700& 2.85     & 5760 & 2.91 \\
R~72~~&5890& 3.19     & 5770 & 3.09 \\
R~79~~&6750& $>$2.94  & 6730 & 3.02 \\
R~83~~&5970& 3.22     & 5770 & 3.07 \\
R~85~~&6390& 3.06     & 6390 & 3.06 \\
R~89~~&4180& 1.60     & 4180 & 1.61 \\
R~92~~&5690& 2.98     & 5630 & 2.93 \\
R~94~~&3950& $\leq$ 0.87 & 3903 & 0.77  \\
R~95A~&5080& 2.99     & 5020 & 2.93 \\
&    &   &   &  \\ \hline
\end{tabular}
\end{flushleft}
\end{table*}


\begin{table}
\caption{Comparison of stars observed in different runs}
\begin{tabular}{ccccr} \hline
 & & & &\\
star & EW(Li) (ESO '94) & H$\alpha$ (ESO '94) & EW(Li) (CTIO) & H$\alpha$ 
(CTIO)\\
   & (m\AA) & (\AA) & (m\AA) & (\AA) \\
 & & & &\\
R~15 & 259 & $+$0.20 & 255 & $+$0.2 \\
R~66 & 186 & $-0.95$ & 173 & $-1.0$ \\
R~70 & 168 & $-1.05$ & 172 & $-1.2$\\ 
 & & & &\\
star & EW(Li) (ESO '95) & H$\alpha$ (ESO '95) & EW(Li) (CTIO) & H$\alpha$ 
(CTIO) \\
   & (m\AA) & (\AA) & (m\AA) & (\AA) \\
 & & & &\\
R~24A & 112 & $+$3.0 & 107 & $+1.9$\\
R~31  & $\leq 55$ & $+4.0$ & $\leq 70$ & $+3.9$\\
R~38  & $\leq 50$ & $+4.9$ & $\leq 100$ & $+11.3$\\
 & & & &\\ \hline
\end{tabular}
\end{table}

\end{document}
