**Table 2:** 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).
$\begin{table} \includegraphics[width=16.5cm]{table2.eps} \end{table}$

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