\begin{table}%t2
\caption{\label{t2}Mean radial velocities, variability, and membership.}
\small%\centerline
 {
\begin{tabular}{cccccccclccccccc}  
\hline  \hline                                                          
&&&&&&&&&&&&& \\[-8pt]
Star   & HD   & $V$   & $\rm \langle RV \rangle$ & err   & $N$   & $P$($\chi^2$) &  var   &  Sp. type   &  $v\sin  i$   &  \multicolumn{3}{c}{Membership}   &  Notes  \\                
   &   & mag   &  \kms   & \kms   &   & \%   & const   &   & \kms   &  RV   &  PM   &  Adop.   & \\ (1)   &  (2)   &  (3)   & (4)   & (5)   & (6)   & (7)   &  (8)   &  (9)   &  (10)   &  (11)   &  (12)   &  (13)   &  (14)  \\  
   \hline      
 W3    & 224515 & \phantom{1}8.4  &  --10.8 & 0.4   & 4   & \phantom{1}97 & c   &  K0III    &  ...   &  n   &  n   &  n   &  \\        
 W4    & 224536 & \phantom{1}9.1  &  \phantom{1}\phantom{1}8.3 & 0.7   & 2   & \phantom{1}21 & c   &  F5V      &  ...   &  m   &  n   &  n   &  \\          
 W8    &        & 10.1  &  \phantom{1}\phantom{1}4.9 & 0.6   & 3   & \phantom{1}21 & c   &  F6III    &  ...   &  m   &  n   &  n   &   \\        
 W9    & 224630 & \phantom{1}5.6  &  \phantom{1}--3.5 & 0.4   & 6   & 100 & c   &  K1II-III &  ...   &  n   &  n   &  n   &  \\          
W23    & 224820 & \phantom{1}8.4  &  \phantom{1}\phantom{1}4.8 & 2.2   & 6   & \phantom{1}27 & c   &  A1V      &  180   &  m   &  m   &  m   &  \\          
W26    & 224862 & \phantom{1}7.1  &  \phantom{1}17.6 & 0.4   & 4   & \phantom{1}65 & c   &  G6III    &  ...   &  n   &  n   &  n   &  \\          
W28    &        & 10.5  &  \phantom{1}\phantom{1}6.7 & 0.6   & 3   & \phantom{1}26 & c   &  F2-6V    &  ...   &  m   &  m   &  m   &  \\          
W32    &        & 11.1  &  \phantom{1}10.7 & 0.7   & 4   & \phantom{1}24 & c   &  G8III    &  ...   &  n   &  ... &  n   &  \\          
W35    & 224948 & 10.0  &  \phantom{1}\phantom{1}7.3 & 0.7   & 3   & \phantom{1}73 & c   &  F0V      &  \phantom{1}42   &  m   &  m   &  m   &  \\          
W36    & 224964 & \phantom{1}9.0  &  \phantom{1}\phantom{1}7.3 & 0.5   & 3   & \phantom{1}23 & c   &  A3V      &  \phantom{1}25   &  m   &  m   &  m   &    \\        
W37    & 224976 & \phantom{1}9.9  &  \phantom{1}\phantom{1}2.2 & 0.5   & 23  & \phantom{1}\phantom{1}0 & v   &  F5V      &  \phantom{1}50   &  m?  &  m   &  m   & 1 \\          
W42    & 224990 & \phantom{1}5.0  &  \phantom{1}\phantom{1}5.5 & 0.7   & 95  & \phantom{1}\phantom{1}0 & v   &  B4-5     &  \phantom{1}28   &  m   &  n   &  n   & 2\\
W47    &        & 10.2  &  \phantom{1}\phantom{1}8.7 & 0.9   & 23  & \phantom{1}\phantom{1}0 & v   &  F2V      &  \phantom{1}34   &  m   &  m   &  m   & 2 \\
W51    & 225047 & \phantom{1}8.4  &  \phantom{1}\phantom{1}6.6 & 2.0   & 5   & \phantom{1}87 & c   &  A0V      &  120   &  m   &  m   &  m   &  \\
W54    &        & 10.4  &  \phantom{1}--4.7 & 0.8   & 4   & \phantom{1}38 & c   &  F1-5IV   &  \phantom{1}43   &  n   &  p   &  n   & 3, 4 \\
W55    &        & 10.7  &  \phantom{1}17.3 & 0.9   & 2   & \phantom{1}43 & c   &  G0       &  ...   &  n   &  n   &  n   & 5 \\
W56    &        & 11.3  &  \phantom{1}\phantom{1}6.1 & 0.6   & 3   & \phantom{1}81 & c   &  F8       &  ...   &  m   &  m   &  m   & 4 \\
W57    &        & 10.4  &  \phantom{1}\phantom{1}7.5 & 6.5   & 17  & \phantom{1}\phantom{1}0 & v   &  F3V      &  \phantom{1}26   &  m?  &  m   &  m   & 2 \\
W58    &        & 10.6  &  \phantom{1}\phantom{1}6.7 & 0.6   & 5   & \phantom{1}89 & c   &  F8V      &  \phantom{1}56   &  m   &  m   &  m   &  \\
W59    & 225099 & \phantom{1}9.4  &  \phantom{1}\phantom{1}8.0 & 0.5   & 2   & \phantom{1}33 & c   &  F5IV-V   &  ...   &  m   &  n   &  n   &  \\
W60    &        & 10.6  &  \phantom{1}\phantom{1}6.7 & 0.5   & 5   & \phantom{1}14 & c   &  F4-6V    &  ...   &  m   &  m   &  m   &  \\
W61    & 225111 & 10.2  &  \phantom{1}13.4 & 8.3   & 27  & \phantom{1}\phantom{1}0 & v   &  F0V      &  \phantom{1}28   &  m   &  m   &  m   & 2 \\
W62    &        & 10.4  &  \phantom{1}18.9 & 0.9   & 2   & \phantom{1}74 & c   &  G6IV     &  ...   &  n   &  n   &  n   &  \\ 
W63    &        & 10.6  &  \phantom{1}\phantom{1}4.6 & 0.4   & 5   & \phantom{1}36 & c   &  F4-6V    &  ...   &  m   &  m   &  m   &  \\
W65    & 225119 & \phantom{1}8.2  &  \phantom{1}31.0 & 1.9   & 9   & \phantom{1}\phantom{1}0 & v   &  B9:      &  \phantom{1}45   &  n   &  p   &  n   &  6 \\
W69    & 225155 & \phantom{1}7.7  &  --19.9 & 0.5   & 2   & \phantom{1}83 & c   &  G6III    &  ...   &  n   &  n   &  n   &  \\
W71    & 225187 & \phantom{1}7.1  &  \phantom{1}\phantom{1}1.9 & 2.8   & 13  & \phantom{1}\phantom{1}0 & v   &  B7       &  150   &  ?   &  m   &  m?  &   \\
W74    &        & 10.5  &  \phantom{1}\phantom{1}6.6 & 0.5   & 10  & \phantom{1}53 & c   &  F6V      &  \phantom{1}53   &  m   &  m   &  m   &  \\          
W75    & 225200 & \phantom{1}6.4  &  \phantom{1}14.9 & 5.0   & 12  & \phantom{1}\phantom{1}0 & v?  &  A2shell  &  300:  &  m:  &  p   &  m?  & 7 \\          
W76    & 225206 & \phantom{1}7.8  &  \phantom{1}\phantom{1}6.0 & 1.8   & 40  & \phantom{1}\phantom{1}0 & v   &  B8V      &  146   &  m   &  m   &  m   &  \\          
W80    &        & 11.0  &  \phantom{1}\phantom{1}7.7 & 0.6   & 5   & \phantom{1}26 & c   &  F6-8     &  ...   &  m   &  m   &  m   &  \\          
W86    & 225264 & \phantom{1}8.3  &  \phantom{1}\phantom{1}5.0 & 3.4   & 16  & \phantom{1}\phantom{1}0 & v   &  A0-A1V   &  \phantom{1}33   &  m   &  m   &  m   & 2 \\          
W88    & 225282 & \phantom{1}8.3  &  \phantom{1}\phantom{1}5.4 & 1.4   & 8   & \phantom{1}86 & c   &  A0-1     &  137   &  m   &  m   &  m   & 3 \\          
W96    &    50  & \phantom{1}9.7  &  \phantom{1}\phantom{1}4.5 & 1.9   & 32  & \phantom{1}\phantom{1}0 & v   &  F0V      &  \phantom{1}40   &  m   &  m   &  m   &  \\          
W104   &    91  & \phantom{1}9.9  &  \phantom{1}\phantom{1}6.8 & 0.5   & 2   & \phantom{1}78 & c   &  F0V      &  ...   &  m   &  m   &  m   & 2 \\          
W106   &  104   & \phantom{1}8.0  &  \phantom{1}--0.3 & 0.6   & 2   & \phantom{1}80 & c   &  G8-K0III &  ...   &  n   &  n   &  n   &  \\          
W109   &  117   & \phantom{1}9.2  &  \phantom{1}15.7 & 0.5   & 4   & \phantom{1}99 & c   &  F4-8     &  ...   &  n   &  n   &  n   &  \\          
W111   &  141   & \phantom{1}7.9  &  \phantom{1}11.4 & 4.4   & 8   & 100 & c   &  B9V      &  204   &  m   &  m   &  m   &  \\          
W121   &  212   & 10.2  &  \phantom{1}\phantom{1}7.7 & 2.1   & 5   & \phantom{1}\phantom{1}1 & ?   &  F3V      &  \phantom{1}94   &  m   &  m   &  m   &  \\          
W124   &  235   & \phantom{1}8.7  &  \phantom{1}\phantom{1}4.9 & 4.3   & 11  & 100 & c   &  A1V      &  218   &  m   &  m   &  m   & 3 \\          
W126   &  343   & \phantom{1}9.8  &  \phantom{1}\phantom{1}7.5 & 5.7   & 3   & \phantom{1}\phantom{1}2 & ?   &  A6       &  155   &  m   &  m   &  m   &  \\          
W128   &  394   & \phantom{1}9.6  &  \phantom{1}\phantom{1}3.9 & 1.1   & 2   & \phantom{1}94 & c   &  F8V      &  \phantom{1}34   &  m   &  n   &  n   &  \\          
E54   &        & 10.1  &  \phantom{1}\phantom{1}5.4 & 0.5   & 3   & \phantom{1}83 & c   &  F0V      &  \phantom{1}28   &  m   &  m   &  m   & 3 \\  
E57   & 225077 & \phantom{1}8.9  &  \phantom{1}\phantom{1}7.5 & 1.2   & 28  & \phantom{1}\phantom{1}0 & v   &  A3V      &  ...   &  m   &  m   &  m   & 2 \\  
E51   &        & 10.3  &  \phantom{1}\phantom{1}5.2 & 1.1   & 3   & \phantom{1}86 & c   &  F5V      &  \phantom{1}86   &  m   &  m   &  m   &  \\ 
\hline
\end{tabular}}                                                      
\medskip
Notes: 1~the location in the color$-$magnitude diagram suggests duplicity (see Fig.~\ref{fig.cmd});
2~binary star with calculated orbit. For kinematic membership~$V_\gamma$ was used;
3~RV~variability inferred from the RV~difference with previous studies (see text);
4~proper motion membership taken from Mermilliod et~al. (\cite{m08});
5~RV~variable in Mermilliod et~al. (\cite{m08}); 
6~suspected SB2 (see text);
7~Shell Star. RV of narrow spectral lines is constant at 6.6~$\pm$ 0.7~\kms.
\end{table}