\begin{table}%t1
\par
\caption{\label{n2682}Radial  and rotational velocities for stars in NGC 2682.}
%\centerline
 {
\begin{tabular}{rlrrrrrrr}
\noalign{\smallskip}\hline\hline\noalign{\smallskip}
\multicolumn{1}{c}{No.} & \multicolumn{1}{c}{ID} & \multicolumn{1}{c}{$V_r$} & 
\multicolumn{1}{c}{$\epsilon$} & $N$ & $V \sin i$ & Err & $\Delta T$ & $P(\chi^2)$ \\
\noalign{\smallskip}\hline\noalign{\smallskip}
0003 & F   3  & 32.51 & 0.63 & 2 &  9.3 & 1.7 & 736 & 0.128  \\
0006 & F   6  & 33.77 & 0.38 & 2 &  6.0 & 2.0 & 736 & 0.814  \\
0018 & F  18  & 32.81 & 0.40 & 2 & 11.2 & 1.4 & 736 & 0.775  \\
0020 & F  20  & 33.45 & 0.31 & 2 &  0.9 & 0.0 & 734 & 0.249  \\
0037 & F  37  & 33.11 & 0.34 & 2 &  2.6 & 2.0 & 697 & 0.251  \\
0048 & F  48  & 32.56 & 0.30 & 2 &  0.4 & 4.4 & 697 & 0.688  \\
0054 & F  54  & 34.72 & 0.36 & 2 &  4.6 & 2.5 & 734 & 0.258  \\
0072 & F  72  & 33.17 & 0.26 & 2 &  1.2 & 2.2 & 735 & 0.985  \\
0094 & F  94  & 33.17 & 0.32 & 3 &  8.1 & 1.4 & 734 & 0.796  \\
0096 & F  96  & 33.75 & 0.34 & 2 &  7.3 & 1.5 & 695 & 0.490  \\
0115 & F 115  & 34.24 & 0.25 & 3 &  3.4 & 2.3 & 734 & 0.801  \\
0127 & F 127  & 33.99 & 0.35 & 3 &  5.3 & 1.6 & 734 & 0.193  \\
0157 & F 157  & 32.86 & 0.36 & 2 &  7.3 & 1.7 & 694 & 0.708  \\
0163 & F 163  & 33.06 & 0.67 & 2 &  5.2 & 1.9 & 694 & 0.045  \\
0166 & F 166  & 32.60 & 0.28 & 2 &  2.9 & 0.0 & 694 & 0.944  \\
0193 & F 193  & 33.94 & 0.26 & 2 &  2.6 & 1.7 & 694 & 0.383  \\
0215 & F 215  & 33.08 & 0.43 & 2 & 10.6 & 1.6 & 694 & 0.641  \\
0226 & F 226  & 33.00 & 0.27 & 2 &  2.0 & 2.0 & 694 & 0.860  \\
0227 & F 227  & 33.03 & 0.31 & 2 &  5.0 & 1.8 & 694 & 0.465  \\
0237 & F 237  & 33.52 & 0.69 & 2 &  0.0 & 0.0 & 695 & 0.015  \\
0241 & F 241  & 32.53 & 0.36 & 2 &  5.2 & 2.1 & 696 & 0.409  \\
0243 & F 243  & 33.09 & 0.36 & 2 &  6.4 & 1.9 & 696 & 0.572  \\
0256 & F 256  & 33.24 & 0.35 & 2 &  6.0 & 3.1 & 696 & 0.739  \\
0271 & F 271  & 34.00 & 0.33 & 2 &  4.5 & 2.2 & 696 & 0.976  \\
0272 & F 272  & 30.16 & 0.56 & 2 &  5.5 & 1.9 & 696 & 0.102  \\
0281 & F 281  & 32.74 & 0.32 & 2 &  5.1 & 1.8 & 696 & 0.322  \\
0287 & F 287  & 32.46 & 0.40 & 2 &  8.3 & 1.7 & 696 & 0.424  \\
0289 & F 289  & 33.18 & 0.50 & 2 &  7.3 & 2.1 & 697 & 0.198  \\
0303 & F 303  & 35.12 & 0.35 & 2 &  4.2 & 2.4 & 697 & 0.365  \\
0317 & F 317  & 33.18 & 0.33 & 2 &  2.2 & 0.0 & 697 & 0.744  \\
4018 & S 1060 & 33.58 & 0.50 & 1 &      &     &     &        \\
7368 & S  368 & 33.82 & 0.35 & 2 &  0.5 & 3.4 & 698 & 0.902  \\
7489 & S  489 & 33.42 & 0.51 & 2 &  8.8 & 2.2 & 699 & 0.829  \\
7657 & S  657 & 32.57 & 0.32 & 2 &  5.7 & 1.7 & 699 & 0.707  \\
7859 & S  859 & 32.07 & 0.45 & 2 &  0.9 & 3.1 & 699 & 0.191  \\
7871 & S  871 & 32.75 & 0.38 & 2 &  5.7 & 2.2 & 699 & 0.580  \\
8524 & S 1524 & 33.04 & 0.57 & 1 &  1.5 & 4.3 &     &        \\
8639 & S 1639 & 32.90 & 0.37 & 2 &  3.8 & 0.0 & 698 & 0.777  \\
8713 & S 1713 & 32.87 & 0.64 & 2 &  4.2 & 1.9 & 698 & 0.031  \\
8792 & S 1792 & 33.67 & 0.36 & 2 &  3.5 & 2.2 & 698 & 0.436  \\
\hline
\end{tabular}}
\par
\smallskip
Note: the star designation corresponds to that used in WEBDA. In the column ID, F refers to Fagerholm (\cite{ef06})
and S to Sanders (\cite{wls77}). The successive columns give:  the radial velocity ($V_r$) and error on the mean ($\epsilon$),
the number of measurements~($N$), the rotation ($V \sin i$) and its error (Err), the time interval covered by the observations
($\Delta T$) and the probability that the scatter is due to random noise ($P(\chi^2)$).
\end{table}