\begin{table}%t2
\par
\caption {Mean radial and rotational velocities for 31 member stars.
\label{mem}}
%\centerline
 {\begin{tabular}{rrrrrlrrrrrrrrrrrl}
\hline\hline%\noalign{\smallskip}
 No. & $V$ & $U-B$ & $B-V$ & $V-I$ & SpT & \multicolumn{1}{c}{$V_{\rm r}$} & \multicolumn{1}{c}{$\epsilon$} & $N$ & $\Delta T$ & $P(\chi^2)$ & $V\sin i$ & rms & $RV_{\rm{lit}}$ & Err & $n$ & Src & Rem \\
\hline%\noalign{\smallskip}
 12 &  9.54 &       & 0.60 &       & G0     & +0.55 & 0.15 & 11 & 6934 & 0.195 &  6.6 & 0.6 & +0.7 & 0.8 & 1 & b &   \\
 19 &  8.12 & --0.02 & 0.39 & 0.477 & F5 V   & +0.69 & 0.29 & 13 & 7536 & 0.069 & 21.7 & 2.2 & --0.1 & 0.6 & 3 & a &    \\
 36 &  8.12 & --0.04 & 0.40 & 0.482 & F3 V   & +0.03 & 0.79 & 12 & 5820 & 0.009 & 35.1 & 3.5 & +0.7 & 1.8 & 3 & a &   \\
 48 &  8.80 &  0.08 & 0.52 &       & F7 V   & --0.43 & 0.14 & 37 & 3565 & 0.000 &  9.6 & 1.4 &      &     &   &   & SB2O   \\
 53 &  8.74 &  0.02 & 0.51 &       & F7 V   & --0.37 & 0.11 & 38 & 5852 & 0.000 &  6.1 & 0.4 & --9.7 & 0.2 & 1 & a & SB1O  \\
 58 &  8.82 & --0.00 & 0.50 &       & F7 V   & +0.40 & 0.16 & 15 & 7271 & 0.441 & 16.0 & 0.4 & +1.5 & 0.1 & 1 & a &   \\
 65 &  9.02 &  0.04 & 0.57 & 0.673 & F5 V   & --0.51 & 0.12 & 16 & 7271 & 0.754 &  9.5 & 0.5 & --2.4 & 1.0 & 1 & d &    \\
 76 &  9.31 &  0.08 & 0.59 & 0.631 & G0 V   & --0.75 & 0.12 & 13 & 7271 & 0.769 &  9.0 & 0.4 & +0.3 & 1.0 & 1 & d &   \\
 85 &  9.31 &  0.06 & 0.59 & 0.653 & G0 V   & +0.15 & 0.12 & 11 & 7271 & 0.976 &  7.8 & 0.5 & +2.6 & 1.0 & 1 & d &   \\
 86 &  8.53 & --0.02 & 0.46 & 0.544 & F7 V   & --0.77 & 0.21 & 13 & 7536 & 0.646 & 20.7 & 2.1 & +1.3 & 0.9 & 2 & a &   \\
 90 &  8.55 & --0.04 & 0.46 & 0.542 & F6 V   & +0.28 & 0.18 & 13 & 7273 & 0.354 & 15.3 & 0.5 & +0.7 & 0.1 & 1 & a &   \\
 92 &  8.68 &  0.02 & 0.53 & 0.697 & F8 V   & --0.23 & 0.15 & 30 & 7540 & 0.305 & 20.8 & 2.1 & --1.5 & 2.1 & 4 & e &   \\
 97 &  9.18 &  0.00 & 0.54 & 0.643 & F8 V   & --0.23 & 0.10 & 64 & 4620 & 0.000 & 17.7 & 0.3 & +3.6 &13.8 & 5 & e & SB1O  \\
101 &  8.38 & --0.03 & 0.45 & 0.521 & F6 V   & --0.16 & 0.42 & 13 & 7273 & 0.034 & 25.3 & 2.5 & --1.2 & 1.3 & 2 & a &     \\
102 &  9.33 &  0.07 & 0.60 & 0.692 & G0 V   & +0.18 & 0.06 & 59 & 6218 & 0.000 &  4.3 & 0.4 & --3.1 & 1.0 & 1 & c & SB1O  \\
114 &  8.58 & --0.05 & 0.45 & 0.539 & F7 V   & +0.77 & 0.18 & 11 & 7272 & 0.974 & 15.5 & 0.4 & --0.7 & 0.1 & 1 & a &   \\
118 &  8.36 & --0.03 & 0.44 & 0.518 & F6 V   & +0.27 & 0.24 & 11 & 7539 & 0.188 & 16.5 & 0.5 & --0.4 & 0.2 & 2 & a &   \\
120 &  9.76 &  0.28 & 0.80 &       & G7     & +1.03 & 0.12 & 26 & 5510 & 0.000 &  6.4 & 0.5 &+12.1 & 1.0 & 1 & d & SB1O   \\
132 &  9.88 &  0.18 & 0.67 & 0.728 & G5 V   & --0.03 & 0.12 & 11 & 7539 & 0.501 &  3.5 & 0.8 & --0.5 & 1.0 & 1 & d &    \\
150 &  9.78 &  0.31 & 0.78 & 0.852 & G9 V   & +0.30 & 0.12 & 29 & 4346 & 0.000 & 12.5 & 2.5 & +0.1 & 0.3 & 1 & a & SB2O  \\
162 &  8.60 & --0.04 & 0.48 & 0.546 & F7 V   & --0.04 & 0.22 & 12 & 7537 & 0.256 & 18.3 & 0.5 & --0.5 & 1.0 & 2 & a &  \\
213 & 10.48 &  0.38 & 0.77 &       & K0 V   & +0.12 & 0.14 &  8 & 5104 & 0.846 &  5.0 & 0.9 & +0.9 & 1.0 & 1 & c & Tr A13  \\
220 & 10.78 &       & 0.89 &       & K0 III & +0.83 & 0.16 &  6 & 3631 & 0.738 &  3.5 & 1.2 & +0.3 & 0.8 & 1 & b & Tr A20  \\
282 & 11.46 &  0.84 & 1.10 &       & K1 V   & --0.01 & 0.20 &  4 & 2834 & 0.969 &  1.4 & 2.8 &      &     &   &   & Argue 9-16  \\
390 &  8.87 &       &      &       & F8 V   & --0.83 & 0.57 &  2 & 2168 & 0.703 & 12.7 & 1.6 & --2.4 & 1.0 & 1 & c & Griffin \\
395 &  9.71 &       & 0.63 &       & G0     & --1.46 & 0.21 &  4 & 2063 & 0.891 &  6.4 & 0.9 & --0.5 & 2.0 & 1 & c & Bou 50 \\
400 &  8.24 &       &      &       & F5 V   & --0.80 & 0.79 &  2 & 1091 & 0.722 & 23.8 & 6.5 &      &     &   &   & Griffin \\
420 & 12.13 &       & 1.20 &       &        & --0.20 & 0.20 &  5 & 4020 & 0.686 &  4.7 & 1.3 &      &     &   &   & Malm 26.155   \\
421 & 11.94 &       & 1.15 &       & K2 V   & --0.69 & 0.25 &  5 & 3688 & 0.153 &  1.0 & 3.6 &      &     &   &   & Malm 26.215  \\
431 & 11.25 &       & 1.00 &       & K0 IV  & --0.10 & 0.18 &  5 & 3697 & 0.846 &  3.8 & 1.9 &      &     &   &   & Malm 28.277  \\
436 &  8.63 &       & 0.59 &       & F8 V   & --1.91 & 0.20 &  8 & 3633 & 0.251 & 14.1 & 0.5 &      &     &   &   & Malm 30.252  \\
%\noalign{\smallskip}
\hline
\end{tabular}}
\par
%\smallskip
Notes: stellar identification, according to Trumpler (\cite{tr38}) and extension in WEBDA, $V$, $B-V$, $U-B$, 
and $V-I_K$~photometric indices, spectral types, CORAVEL mean radial velocities and errors in km~s$^{-1}$, the number of observations, 
probabilit~$P(\chi^2)$ that the scatter is due to random errors, projected rotation ($V\sin i$) and error, also in km~s$^{-1}$,
radial velocities from the literature, their error and sources, and remarks on binarity and cross-identifications. 
Literature sources: 
a: Kraft (\cite{rpk65}); 
b: Glushkova (\cite{eg93}); 
c: Ford et~al. (\cite{fjjb01}); 
d: Jeffries (\cite{rdj99}) ; 
e: Trumpler (\cite{tr38}).
\end{table}