\begin{table}%t1
\caption {\label{tab_HVS}Results of the spectroscopic and kinematic analysis of J0136+2425.}
%\centerline
 {\begin{tabular}{lc|lc}
\hline\hline
$V$ (mag)$^{a} $     & 16.17 $\pm$ 0.02 & 
$E(B-V)$ (mag)$^{b} $ &  0.16 $\pm$ 0.02 \\
$\mu_\alpha\cos(\delta)$~(\masyr) &   $-$2.2 $\pm$ 1.3 & 
$\mu_\delta$~(\masyr) &   $-$8.2 $\pm$ 2.2 \\
\teff\ (K)      &  9100 $\pm$ 250  & 
 \logg (cgs)      &  3.90 $\pm$ 0.15  \\
 \M          &  0.0             &  
 $M/M_\odot$ &  2.45 $\pm$ 0.20   \\
 $v_{\rm rad}$ (\kms)   & 324.3 $\pm$ 5.9 &
 $v_{\rm rot} \sin i$ (\kms) & 250 \\ 
 $d$ (kpc)    & 10.90 $\pm$ 2.00  &    
 $v_{\rm grf}$ (\kms) & $\rm 587 ^{+144}_{-89}$   \\
 $v_{\rm ej}$ (\kms)  & 551                 & 
 $v_{\rm esc}$ (\kms) & 466                  \\
 TOF (Myr)           &  12 $\pm$ 1.3  & $t_{\rm evol}$ (Myr) & 245    \\
 \hline
 \end{tabular} }
\par
 \smallskip
 {$^{a}$ The visual magnitude 
derived following \cite{2006AetA...460..339J}};
 {$^{b}$ The interstellar colour excess $E(B-V)$ was determined}
 {by comparing the observed colours to synthetic ones}
 {from the model spectral energy
\mbox{distribution}. }
\end{table}