\begin{table}%t2
\caption{\label{Tab:Sb}Binaries inferred from the high rotational velocity of the giant primary.}
%\centerline
 {\small \begin{tabular}{rrllllllllp{6cm}}
\hline \hline
HD  & HIP & SB?$^a$  & $\sigma_0$ & $Sb$ &  $V \sin i$ & $V-I$  & $T_{\rm eff}$  & $M_V$  & $R$  & Rem\\
    &     &      & (\kms) & (\kms) & (\kms) & & (K) & & ($R_{\odot}$) \\
\hline
10696 & 8175 & -- & -- & 10.5 &  -- & 2.3  & 3590 & 0.51 & 43 & not a fast rotator; $Sb$ contaminated by close (0.16'') visual companion\\
190658& 98954 & y & 8.7 & 8.5 &   10 & 2.1 & 3670 & $-0.67$ & 63   & Ellipsoidal variable, spectroscopic binary with $P = 199$ d\\
219654 & 114985 & y & 6.1 & 7.7 & 14 & 1.9 & 3730 & -- & --   & not listed in Table~4b of Paper~I because it only belongs to sample~I\\
\hline
\end{tabular}}
\medskip
$^a$ This column provides the diagnostics of spectroscopic binarity based on the location of the star in the $Sb - \sigma_0(V{\rm r})$ diagram (Fig.~\ref{Fig:Sb-sigma}); HD~219654: SB: JD~2\ts448\ts843.634:~$5.22\pm 0.4$~\kms,  JD 2\ts449\ts676.270:   $13.84\pm 0.3$~\kms.
\end{table}