\begin{table}%t1
\caption{\label{tab1}Basic model properties: sequence number,  
$M_{\rm init}$: initial mass, $Z$: metallicity, 
$\dot M_{{\rm WR}}$: option for the WR~wind mass loss rate, 
$f_{\rm K}$: initial rotational velocity in units of the Keplerian value, 
$V_{\rm init}/V_{\rm crit}$: the ratio of the initial rotational velocity to the critical velocity at the equator (Eq.~(4)), 
$Y_{\rm s, H-end}$: surface helium abundance at core hydrogen exhaustion, 
$M_{\rm final}$: final mass, 
$M_{\rm CO}$: CO~core mass at core carbon exhaustion,  
$J_{\rm init}$: initial angular momentum, 
$J_{\rm final}$: final angular momentum, 
$j_{3~M_\odot}$: mean specific angular momentum in the innermost $3\mso$,
$X_{\rm N, max}$:
maximum nitrogen surface mass fraction during the evolution.
}
%\centerline
{
\begin{tabular}{lccccccccccccc} 
\hline
\hline
No. & $M_{\rm init}$ & $Z$ & $\dot M_{{\rm WR}}$  &$V_{\rm init}$ & $f_{\rm K}$ & $V_{\rm init}/V_{\rm crit}$   & $Y_{\rm s, H-end}$ & $M_{\rm final}$ & $M_{\rm CO}$ &   
$J_{\rm init}$ & $J_{\rm final}$ & $j_{3~M_\odot}$ & $X_{\rm N, max}$ \\
    & [${M_\odot}$] &  &   & [${\rm km~s^{-1}}$]  &  &  & &    [${M_\odot}$] &  [${M_\odot}$] &   
[$10^{51}$ & [$10^{51}$  & [$10^{15}$  &   \\ 
&&&&&&&&&& erg s] & erg s]& ${\rm cm^2~s^{-1}}$]&\\
\hline
A1  & 20 & $10^{-5}$ & WR1  &479 & 0.5 & 0.56   & 0.94   & 16.40  & 9.48  & 46.92  &  3.79 & 2.50 & $2.6\times 10^{-6}$ \\
A2  & 30 & $10^{-5}$ & WR1  &501 & 0.5 & 0.58   & 0.94   & 24.13  & 18.80  & 98.80  &  8.40 & 10.57 & $1.3\times  10^{-2}$ \\
A3  & 40 & $10^{-5}$ & WR1  &230 & 0.2 & 0.25   & 0.27   & 39.84  & 7.08   & 73.58  & 65.36 & 0.90  & $4.2\times  10^{-6}$\\
A4  & 40 & $10^{-5}$ & WR1  &555 & 0.5 & 0.60   & 0.94   & 31.77  & 25.23  & 166.21 & 12.57 & 12.57 & $1.4\times  10^{-2}$ \\
A5  & 50 & $10^{-5}$ & WR1  &583 & 0.5 & 0.64   & 0.94   & 39.21  & 33.68  & 247.54 & 19.03 & 13.75 & $3.2\times  10^{-2}$ \\
A6  & 60 & $10^{-5}$ & WR1  &605 & 0.5 & 0.63   & 0.94   & 46.50  & 40.25  & 341.70 & 23.55 & 13.41 & $2.8\times  10^{-2}$ \\
\hline
B1  & 40 & $0.001 $  & WR1  &479 & 0.5 & 0.63  & 0.90   & 13.52  & 10.70  & 183.97 & 0.21  & 0.82  & $6.7\times  10^{-4} $ \\
B2$^*$  & 40 & $0.02 $   & WR1  &408 & 0.5 & 0.69  & 0.69   & 20.25  &  --    & 166.40 & 1.505 &  3.30 & $1.3\times  10^{-2}$ \\
\hline
C1  & 40 & $0.001 $  & WR2  &479 & 0.5 & 0.63  & 0.96   & 25.71  & 21.23  & 183.97 & 8.94  & 12.92 & $3.3\times  10^{-3}$\\
C2  & 60 & $0.001 $  & WR2  &522 & 0.5 & 0.67  & 0.96   & 34.59  & 30.18  & 378.32 & 10.12 & 9.88  & $6.7\times  10^{-4}$\\
\hline
\end{tabular}}
\smallskip
$^*$ sequence ends at core hydrogen exhaustion.
\end{table}