\begin{table}%T1
%\renewcommand{\arraystretch}{1.2}
%\centering
\par
\caption{Properties of the computed models. The first column denotes 
the sequence number, where "NR'', "R'' and "RT'' denote
the non-rotating models and rotating models with $f_{\rm c} = 1/30$ and 1/3 respectively. 
The second column gives the accretion rate in units of $10^{-7}$~\msyr. 
The third column denotes the factor $f_{\rm c}$ for the chemical mixing efficiency in rotating models.
Columns~4--7 give mass, central density, central temperature and \TW{} of the last computed model 
of each evolutionary sequence. The eighth column gives the amount of accreted
material until the onset of the helium shell instability.
The column with $L_{\rm Edd}$ indicates whether the last computed model reached the Eddington limit or not.
The last column gives the total number of the computed models for each sequence.
}\label{tab1}
\begin{tabular}{c c c c c c c c c r}
\hline \hline\\[-3.2mm]
No.  & \Mdot{} & $f_{\rm c}$& $M_{\rm last}$ & $\rho_{\rm c, last}$ & $T_{\rm c, last}$ & $(E_{\rm rot}/|E_{\rm grav}|)_{\rm last}$ & $\Delta M$ &  $L_{\rm Edd}$ &  No. of models   \\
     & [$10^{-7}$~\msyr]   &    &   [\Msun]         &     [$10^8~{\rm g/cm^3}$]  & [$10^8$ K] &   & [\Msun] &  \\[-3.2mm]\\
\hline
NR1  & 2.0 & -- & 1.0026 & 0.25 & 1.45 & -- & 0.00 & Yes & 4342  \\
NR2  & 3.0 & -- & 1.0042 & 0.25 & 1.45 & -- & 0.00 & Yes & 5164 \\
NR3  & 5.0 & -- & 1.0130 & 0.28 & 1.37 & -- & 0.00 & Yes & 10~324 \\
NR4  &  10 & -- & 1.1984 & 1.39 & 1.44 & -- & 0.03 &  No & 383~637  \\
\hline
R1   & 2.0 & 1/30 & 1.0074 & 0.28 & 1.25 & 0.0018 & 0.00 & Yes & 18~021 \\ 
R2   & 3.0 & 1/30 & 1.0224 & 0.32 & 1.17 & 0.0025 & 0.00 & Yes & 28~449 \\
R3   & 5.0 & 1/30 & 1.2241 & 1.05 & 1.21 & 0.0197 & 0.14 &  No & 180~004\\
R4   &  10 & 1/30 & 1.4773 & 5.14 & 1.72 & 0.0578 & 0.48 &  No & 490~026\\
RT1   & 2.0 & 1/3 & 1.0665 & 0.42 & 0.99 & 0.0081 & 0.01 &  No & 174~270\\
RT2   & 3.0 & 1/3 & 1.1537 & 0.77 & 1.22 & 0.0080 & 0.01 &  No & 212~730\\
\hline
\end{tabular}
\end{table}