\begin{table}%t5
%\centering
\par
\caption{Heliocentric radial velocity (with its standard error) of the
program stars, binary status and cluster membership according to radial
velocities, and projected rotational velocity (with its standard error). The
radial velocity of the binary stars is the barycentric velocity from the
orbital solutions in Table~\ref{t6}. The last column gives the projected rotation
period $P_{\rm rot}$/$\sin i$ of the solved binaries to be compared with the
orbital period.}\label{t5}
\par
\begin{tabular}{rccccc}
\hline
\hline
\#     & $RV_{\odot}$      & binary & member& {$V_{\rm rot}\sin i$}& $P_{\rm rot}$/$\sin i$\\
       & (km s$^{-1}$)     &        &       &  {(km s$^{-1}$)} & (days) \\
\hline
1      & $  +8.6\pm0.5$ & yes & no  & $26\pm1$ & 5.0 \\	
2      & $  -17\pm6  $ & yes & yes & $128\pm3 $ & 10 \\
3      & $-18.5\pm0.6$ & yes & yes & $84\pm2$ & 15 \\
4      & $-15.0\pm0.6$ & yes & yes & $103\pm2 $ & 10 \\
5      & $-19.4\pm0.3$ & no  & yes &	         &    \\
6      & $-25.6\pm0.9$ & yes &(yes)& $253\pm5$  &    \\
7      & $  -18\pm3  $ & yes & yes & $46\pm5$ & 3.8\\
8      & $-15.5\pm0.4$ & no  & yes & $67\pm2$ &    \\
9      & $-5.6 \pm0.5$ & no  & no  & $22\pm2$ &    \\
10     & $-14.8\pm0.7$ & no  & yes & $64\pm7$ &    \\
11     & $     0\pm3 $  & yes & no  & $41\pm6$ & 11 \\
12     & $  -17\pm6 $  & yes & yes & $165\pm7$  & 1.5\\
13     & $-14.6\pm0.2$ & no  & yes & $~0\pm2 $&    \\
14     & $-19.9\pm0.4$ & no  & yes & $11\pm3 $&    \\
15     & $  -16\pm2  $ & no  & yes & $115\pm4 $&    \\
16     & $  -27\pm4  $ & yes &(yes)& {$325\pm20$}&    \\
\hline
\end{tabular}
\end{table}