\begin{table}%t1
\par
\caption{The properties of the three star-forming dwarf galaxies in the Virgo cluster under study.  
\label{t1}}
%\centering
\par
\begin{tabular}{lccccccc}
\hline \hline\noalign{\smallskip}
ID &   $m_{\rm B}$    &12 + log(O/H) &  $SFR$  &    log($M_{\rm HI}/M_{\odot}$) & $T_{\rm d}^{\rm 1BB}$ & log($M_{\rm d}/M_{\odot}$) &  log(\D)\\
 &  mag  & &\msun yr$^{-1}$ &    &  K  &    & \\
\hline 
\object{VCC~562}    &  16.74     &    $7.8\pm0.2$    &   4.6 $\times 10^{-2}$ & $7.67\pm0.03$  & $20.2\pm0.2$ &  $5.18\pm0.13$ & --$2.49\pm0.13$ \\
\object{VCC~1179}    &  15.46     &   $ 8.3\pm0.2$    &   9.4 $\times 10^{-2}$ & $7.39\pm0.06$  & $16.2\pm0.6$ &  $5.48\pm0.14$ & --$1.91\pm0.15$  \\
\object{VCC~1356}    &  16.15     &    $8.0\pm0.3$    &   4.6 $\times 10^{-2}$ & $8.35\pm0.01$  & $17.9\pm1.1$ &  $5.53\pm0.16$ & --$2.82\pm0.16$ \\
\hline 
\end{tabular}
\par
\tablefoot{Dust temperature, masses, and dust-to-gas ratios were obtained by fitting a single modified black-body function with $\beta = 2$. The distance to Virgo is assumed to be 16.5 Mpc.}
\end{table}