\begin{table}%t3
\caption{Fate of the disk mass at the end of each run: results for
scenarios without ($\nrightarrow$) and with ($\rightarrow$) type~I migration.}\label{table:3}  
%\centering
\small
\begin{tabular}{c| c c| c c| c c}
 \hline\hline  
Scenario & I$\nrightarrow$ & I$\rightarrow$ & IV$\nrightarrow$ & IV$\rightarrow$ & V$\nrightarrow$ & V$\rightarrow$\\
 \hline\hline  
Total initial solids $({M}_{\oplus})$ & 24.81 & 24.81 & 24.81
& 24.81 & 24.81 & 23.47\\
 \hline 
Total surviving solids $({M}_{\oplus})$ & 16.60~(67\%) &
18.70~(75\%) & 21.23~(86\%) & 15.13~(61\%) & 20.22~(81\%) &
18.23~(78\%)\\
 \hline 
Interior surviving solids $({M}_{\oplus})$ & 0.88~(4\%) &
3.44~(14\%) & 0.84~(3\%) & 1.84~(7\%) & 0.31~(1\%) & 6.23~(27\%)\\
$N, f_{{\rm proto}}$ & 0, 0 & 1, 0.99 & 0, 0 & 1, 0.96 & 0, 0 & 1, 1\\
 \hline  
Exterior surviving solids $({M}_{\oplus})$ & 15.72~(63\%) &
15.27~(62\%) & 20.39~(82\%) & 13.29~(54\%) & 19.90~(80\%) & 12.00~(51\%)\\
$N, f_{{\rm proto}}$ & 39, 0.27 & 34, 0.22 & 31, 0.63 & 9, 0.34 &
23, 0.66 & 7, 0.24\\
 \hline  
Accreted by star $({M}_{\oplus})$ & 0.01~(0.04\%) & 0.0~(0\%)
& 0.0~(0\%) & 0.0~(0\%) & 0.0~(0\%) & 0.01~(0.04\%)\\
 \hline  
Accreted by giant $({M}_{\oplus})$ & 8.20~(33\%) &
6.01~(24\%) & 3.41~(14\%)
& 9.68~(39\%) & 4.59~(19\%) & 5.23~(22\%)\\
 \hline 
Ejected $({M}_{\oplus})$ & 0.00~(0\%) & 0.1~(0.4\%) &
0.17~(1\%) &
0.0~(0\%) & 0.0~(0\%) & 0.0~(0\%)\\
 \hline
\end{tabular}
\end{table}