All Tables

Table 1: Case-2a parameters for a binary system of initially $7+1.5~M_{\odot}$ stars with $P_{\rm orb}=350$ d and $\alpha _{\rm CE}=3.0$ . Roche lobe overflow during helium shell burning is allowed post-CE.
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).