\begin{table}%t1
\caption{\label{tab-hydro}Summary of  hydrodynamical results.}
%\centerline
 {\begin{tabular}{cccccccccccccc}
\hline
\hline
\noalign{\smallskip}
 Run & $M_{\rm WD}$ 
     & $M_{\rm disk}$ 
     & $M_{\rm acc}$ 
     & $M_{\rm ej}$ 
     & $T_{\rm peak}$
     & $T_{\rm max}$
     & $R_{\rm disk}$
     & $H$
     & $\Delta t$
     & $E_{\rm nuc}$
     & $E_\nu$
     & $E_{\rm GW}$
     &$\omega$\\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
0.3+0.5 & 0.62 & 0.18 & 0.12 & $10^{-3}$ & $6.0\times 10^8$    & $6.0\times 10^8$  &  0.2  & $6.1\times10^{-3}$ & 300 & $1\times10^{42}$ & $4\times10^{21}$ & $9\times10^{38}$ & 0.14\\
0.4+0.8 & 0.92 & 0.28 & 0.12 & $10^{-3}$ & $6.5\times 10^8$    & $6.0\times 10^8$  &  0.2  & $6.0\times10^{-3}$ & 166 & $1\times10^{44}$ & $5\times10^{24}$ & $4\times10^{39}$ & 0.23\\
0.6+0.6 & 1.10 & 0.10 & 0.50 & $10^{-3}$ & $6.3\times 10^8$    & $6.2\times 10^8$  &  0.07 & $5.5\times10^{-3}$ & 514 & 0                & $3\times10^{24}$ & $1\times10^{41}$ &0.27\\
0.6+0.8 & 1.10 & 0.30 & 0.30 & $10^{-3}$ & $1.6\times 10^9$    & $8.7\times 10^8$  &  0.2  & $5.0\times10^{-3}$ & 164 & $1\times10^{41}$ & $3\times10^{28}$ & $6\times10^{40}$ &0.33\\
0.6+1.2 & 1.50 & 0.30 & 0.30 & $10^{-3}$ & $1.0\times 10^{10}$ & $1.0\times 10^9$  &  0.2  & $4.4\times10^{-3}$ & 122 & $2\times10^{44}$ & $8\times10^{36}$ & $5\times10^{40}$ &0.52\\
\hline
\end{tabular}}
\par
\smallskip
Note: masses and radii  are in solar units, times in seconds
          and  energies  in ergs.   The  maximum temperature  achieved
          during each simulation,  $T_{\rm peak}$, and the temperature
          of the  hot corona formed around  the primary at  the end of
          the  simulations,  $T_{\rm   max}$,  are  discussed  in  the
          text. The rotational velocity is expressed in~s$^{-1}$.
\end{table}