\begin{table}%T1
\par
\caption{\label{ini-abu}Computed late time~(A,~B) and adopted~(C) gas-phase abundances
with respect to~H$_2$ for the
main S-bearing
molecules prior to mantle evaporation.}
%\centerline
{
         \begin{tabular}{l|c|c|c}
\hline\hline
Species & A & B & C \\
\hline
SO     & $9\times 10^{-9}$  & $3\times 10^{-9}$ & $3.1\times 10^{-9}$\\
SO$_2$ & $4\times 10^{-10}$ &$1.5\times 10^{-10}$ & $1\times
10^{-9}$$^{a}$\\
H$_2$S & $1\times 10^{-10}$ & $1\times 10^{-11}$ & $8\times 10^{-10}$\\
CS     & $4\times 10^{-10}$ & $2\times 10^{-8}$ & $1.7\times 10^{-9}$\\
\hline
\end{tabular}}
\smallskip
$^{a}$ Here we took the value of the upper limit.
\end{table}