\begin{table}%T2
\caption{Case-2b parameters for a binary system of initially $7+1.5~M_{\odot}$ stars with $P_{\rm orb}=350$ and $\alpha_{\rm CE}=3.0$. No roche lobe overflow takes place during helium shell burning post-CE because of the high mass-loss rate similar to that proposed by Tout and Hall (1991).}\label{tab2}
    \includegraphics[width=16.5cm]{table2.eps}
    \end{table}