\begin{table}%t7
\caption{Lithium abundances for the stars in IC~4651, computed with both 
spectroscopic~(S) and photometric~(P) values of \teff, assuming a reddening of 
$E(b-y)$~= 0.091; we use the latter in our analysis. Asterisks indicate that~$W$(Li) (in~m\AA) refers to the unblended Li~line. }\label{tab7}
%\centering
\par
\begin{tabular}{lccrrr}
\hline \hline 
Star  & $T$(S)  & $T$(P) & $W$(Li) & $\log~N$(Li)(S) & $\log~N$(Li)(P) \\
\hline
E12   & 5000 & 5020  &   $<$$5$   & $<$$0.35$ & $<$$ 0.38$ \\
E8    & 4900 & 4950  &   $<$$5$   & $<$$ 0.09$ & $<$$ 0.23$ \\
E98   & 4900 & 4950  &   $16 *$ &   0.72 &   0.82 \\
E60   & 4900 & 4930  &    $9 *$ &   0.42 &   0.53 \\
E812  & 5000 & 4910  &   $<$$5$   & $<$$ 0.38$ & $<$$ 0.21$ \\
E95   & 5800 & 5670  &   $35 *$ &   2.19 &   2.07 \\
E3    & 6550 & 6550  &    9   &   1.64 &   1.64 \\
E56   & 6500 & 6520  &   $<$$10$  & $<$$ 2.15$ & $<$$ 2.16$ \\
E19   & 6500 & 6280  &   $<$$5$   & $<$$ 1.83$ & $<$$ 1.66$ \\
E99   & 6800 & 6830  &   $<$$10$  & $<$$ 2.36$ & $<$$ 2.38$ \\
E25   & 6900 & 6680  &   75   &   3.44 &   3.29 \\
E5    & 7100 & 6930  &   76   &   3.59 &   3.47 \\
T1228 & 6800 & 6770  &   58   &   3.20 &   3.18 \\
E14   & 6800 & 6860  &   $<$$5$   & $<$$ 2.03$ & $<$$ 2.07$ \\
E34   & 6850 & 6640  &   $<$$5$   & $<$$ 2.07$ & $<$$ 1.92$ \\
E15   & 6850 & 6540  &   $<$$6$   & $<$$ 2.15$ & $<$$ 1.93$ \\
E79   & 6650 & 6620  &   $<$$5$   & $<$$ 1.93$ & $<$$ 1.91$ \\
E64   & 6650 & 6550  &   $10 *$ &   2.24 &   2.17 \\
E86   & 6600 & 6459  &   $10 *$ &   2.20 &   2.13 \\
T2105 & 6350 & 6138  &   $67 *$ &   3.02 &   2.84 \\
E7    & 6300 & 6308  &   $53 *$ &   2.83 &   2.84 \\
E45   & 6350 & 6103  &   $47 *$ &   2.80 &   2.59 \\
\hline 
\end{tabular}
\end{table}