\begin{table}%t1
%\centering
\par
\caption{\label{tab.inim}Initial models~M \& SC.}
\begin{tabular}{llllllllllllll} 
\hline \hline\noalign{\smallskip}
Model & $M$ & Pop. & $Z$ & $M_{\rm He}$ & $R_{\rm He}$ & $E_{\rm B}$/$k_{\rm B}T$ & $\Gamma_{\rm cnv}$ & $\Psi_{\rm cnv}$ & $L_{\rm He}$ & $L_{\rm H}$   & $T_{\max}$  & $r_{\max}$ & $\rho_{\max}$ \\ 
& $[\Msun]$ & & & $[\Msun]$ & $[10^9\cm]$ & & &&
$[10^9~\Lsun]$  & $[10^9~\Lsun]$ & $[10^8\K]$ & $[10^8\cm]$ & $[10^5\gcm]$  \\
\hline
M  & $1.25$ & I & $0.02$ & $0.47$ & $1.91$ & $<$0.006 & 0.3 & 5 & $1.03$ 
  & $10^{-6}$ & $1.70$ & $4.71$ & $3.44$ \\
\hline 
SC  & 0.85 & III & $0.00 $ & $0.5$ & $5.45$  & $<$0.016 & 0.1 & --2 & $0.004$  
  & 0.07 & $2.04$ & $11.$ & $0.08$  \\
\hline
\end{tabular} 
\tablefoot{Total mass $M$, stellar population, metal content~$Z$, mass $M_{\rm He}$ and radius $R_{\rm He}$ of the helium core, ratio of the binding energy of the electrons $E_{\rm B}$ in the helium core and of their thermal energy $k_{\rm B} T$, ratio of the Coulomb and thermal energy of the ions $\Gamma_{\rm cnv}$, electron degeneracy parameter in the convection zone $\Psi_{\rm cnv}$, nuclear energy production rate due to helium $L_{\rm He}$ and hydrogen $L_{\rm He}$ burning, temperature maximum $T_{\max}$, and  radius $r_{\max}$ and density $\rho_{\max}$ at the temperature  maximum.}
\end{table}