\begin{table}%t7
\caption{\label{tab:subcomp}Properties of the confirmed comoving substellar companions discovered
in the young, nearby associations: TW Hydrae (TWA),~$\beta$ Pictoris
($\beta$ Pic), Columba (Col) and Carina (Car). }
\par
%\centerline
{
\begin{tabular}{llllllllll}
\hline\hline
Name              &      Grp            &  Age       &   $d$                     &  SpT$_{\rm A}$       &  SpT$_{\rm B}$       &   $M_{\rm B}$                  &   $T^B_{\rm{eff}}$  &  $q_{\rm B/A}$  & $\Delta_{\rm proj}$ \\
                  &                     &  (Myr)     &   (pc)                  &                &                &  ($ {M}_{\rm{Jup}}$)   & (K)                 &         &  (AU)        \\ 
\hline
TWA5              &  TWA                &  8         & (45-50)                    
& M1.5           & M8.5           & $25\pm5$                 &    $2500\pm150$     & 0.055   & $93\pm10$       \\
HR7329            &  $\beta$ Pic        &  12        & $\rm 48.2^{+1.8}_{-1.6}$    & A0V            & M8             & $25\pm5$                 &    $2550\pm150$     & 0.010   & $199\pm10$    \\ 
GSC-08047-00232          &  Tuc-Hor/Col    &  30        & (85-95)                    & K3V            & $M9^{\rm +1}_{-3}$ & $20\pm5$                 &    $2100\pm200$     & 0.025   & $295\pm30$    \\
AB Pic            &  Tuc-Hor/Car        &  30        & $\rm 46.0^{+1.6}_{-1.5}$    & K2V            & $L1^{\rm +2}_{-1}$ & $13\pm2$                 &    $1700\pm200$     & 0.015   & $250\pm10$    \\
2M1207            &  TWA                &  8         & $\rm 52.4^{+1.1}_{-1.1}$    
& M8             & late-L         & $4\pm1^*$                  &    $1150\pm150^*$     & $0.16^*$    & $40\pm2$      \\   
%                  &                     &            &                         &                &                & $8\pm2$                  &    $1600\pm100$     & 0.32    &                \\   
\hline
\end{tabular}}
\par
\medskip
-- ($^*$): For 2M1207~b, Mohanty et~al. (\cite{Mohanty07}) suggest a higher mass of
$8\pm2~M_{\rm{Jup}}$ and the existence of a
circum-secondary edge-on disk to explain their measured effective
spectroscopic temperature of $1600\pm100$~K.  (See discussion in Sect.~5.3.3.)
\end{table}