\begin{table}%t3
\caption{\label{table:casos} Input parameters  for cases J1, J3 and J7 of P96$^{{a}}$. }
%\centerline
 {\begin{tabular}{l l l l l l l }
\hline\hline
Case & $\Sigma$ & $\rho$ & $T$ & $r_{\rm p}$ & $t_{\rm cross}$ & $M_{\rm cross}$ \\
    & [g ${\rm cm^{-2}}$] & [g ${\rm cm^{-3}}$] & [K] & [km] & [My] & [${M_{\oplus}}$] \\
\hline
J1 & 10 &  $5 \times 10^{-11}$ &  150 & 100 &7.58 & 16.17\\
J3 & 15 &  $5 \times 10^{-11}$ &  150 & 100 &1.51 & 29.61\\
J7 & 10 &  $5 \times 10^{-11}$ &  150 & 1 &6.94 & 16.18\\
\hline 
\end{tabular}}
\par
\smallskip
 $^{{a}}$ {Here $\Sigma$ is the solids surface density of the disc, $\rho$ is the nebular density, $T$ is the nebular temperature (all at the position of Jupiter) and $r_{\rm p}$ is the radius of accreted planetesimals. The results of P96 for $t_{\rm cross}$ and $M_{\rm cross}$ are also listed.}
\end{table}