\begin{table}%T5
\par
\caption{\label{table4}Final core masses at the pre-supernova stage for different 
models of rotating stars at solar metallicity. 
Note that we use~$M_{\rm{Si}}$ at the end of central Si-burning 
for the value of~$M_{\rm{Fe}}$
as discussed in the text.}
%\centering
\par
\begin{tabular}{l | r r r | r r r | r r}
\hline \hline 
$M_{\rm{ZAMS}}$    &   15   &F15B (HLW)&E15 (HLW)&20    &F20B (HLW)&E20 (HLW)&  25   &E25 (HLW) \\
\hline
$M_{\rm{total}}$   & 10.316 & 12.89 & 10.86  & 8.763 & 14.76 & 11.00  & 10.042 &  5.45         \\
$M_{\alpha}^{01}$  &  5.604 &  3.88 &  5.10  & 8.567 &  5.99 &  7.71  & 10.042 &  5.45         \\
$M_{\rm{CO}}^{01}$ &  3.325 &  2.01 &  3.40  & 5.864 &  2.75 &  5.01  &  7.339 &  4.07         \\
$M_{\rm{Fe}}^{50}$ &  2.036 &  1.38 &  1.46  & 2.245 &  1.36 &  1.73  &  2.345 &  1.69         \\
\hline
\end{tabular}
\end{table}