\begin{table}%t4
  \caption{Main characteristics of computed models representative of~\rvari\ for the two~rotational velocities considered. Labels~$i$ from~0 to~4 indicate the location of the models in the HR~diagram given in Fig.~\ref{fig:HR-rvari}. From left to right, $\Omega$~represents the rotational velocity in~$\kms$, $M$~the stellar mass in solar masses~$\msol$, $\teff$~the effective temperature in~K (on a~logarithmic scale), $g$~the surface gravity in~cgs (on a~logarithmic scale), $X_{\rm c}$~the central Hydrogen fraction, the age in~Myr, $\nuf$~the frequency of the fundamental radial mode (in~$\mu{\rm Hz}$), and finally, $\nu_\Omega$~represents the rotational frequency (in~$\mu{\rm Hz}$) of the model.}\label{tab:rotmodels}
%\centering
\small
    \begin{tabular}{ccccccccccc}
      \hline
      \hline
      & ID & $M$ & $\teff$ & $g$ & $L$ & $\xc$ & Age & $\nuf$ & $\nu_\Omega$ \\
      \hline
 $\Omega=18$ &  &  &  &  & &  & &  & &   \\
     & 02 & 1.75 & 3.859 & 3.94 & 1.13 & 0.304 & 1182 & 130.85 & 1.8 \\
     & 12 & 2.10 & 3.868 & 3.70 & 1.48 & 0.135 & 858  & 82.00  & 1.3 \\
     & 22 & 2.00 & 3.850 & 3.70 & 1.39 & 0.126 & 994  & 82.26  & 1.3 \\
     & 32 & 1.57 & 3.867 & 4.19 & 0.86 & 0.542 & 834  & 208.33 & 2.5 \\
     & 42 & 1.49 & 3.850 & 4.20 & 0.76 & 0.554 & 920  & 202.46 & 2.6 \\
 $\Omega=52.6$ & &  &  &  & &  & &  & &   \\
     & 02 & 1.76 & 3.859 & 3.94 & 1.14 & 0.305 & 1162 & 129.09 & 5.2 \\
     & 12 & 2.10 & 3.868 & 3.70 & 1.48 & 0.141 & 854  & 82.18  & 3.6 \\
     & 22 & 2.01 & 3.850 & 3.69 & 1.40 & 0.127 & 980  & 81.36  & 3.7 \\
     & 32 & 1.58 & 3.868 & 4.19 & 0.87 & 0.543 & 815  & 210.00 & 7.3 \\
     & 42 & 1.49 & 3.850 & 4.20 & 0.76 & 0.560 & 890  & 203.33 & 7.6 \\
      \hline
    \end{tabular}
\end{table}