\begin{table}%t1
\caption{\label{Tab:deltamubinaries}Supplementary ``proper-motion binaries'' found in sample~I using the  method described in \protect\citet{Frankowski-2007} and extracted from their Table~2.}
%\centerline
 {\small \begin{tabular}{lll}
\hline \hline 
HD/BD & HIP & Rem.  \\  
\hline 
5006 & 4100 & SB$^a$ \\
+58 501  & 12~416 & supergiant \\
51802 & 37~391  \\
52554 & 33~929  \\
96572 & 54~571 & SB$^a$ \\
103945 & 58~377 \\
108907 & 60~998 & SB$^a$ ($P = 1714$~d)\\
130218 & 72~268 \\
162159 & 87~114 \\
190658 & 98~954 & SB$^a$ ($P = 198.7$~d)\\
       &       & +visual companion at 2.3$''$ \\
+39 4208 & 101~023 & supergiant\\
199871 & 103~528 & SB$^a$ ($P = 840$~d)\\
209026 & 108~588 \\
219981 & 115~191 \\
220088 & 115~271 & SB$^a$ ($P = 2518$~d)\\ 
\hline 
\end{tabular}}
\medskip
$^a$ The star is also flagged as spectroscopic binary from the radial-velocity data.
 \end{table}