\begin{table}%T2
%\centering
\par
    \caption{Table containing the main characteristics of $M=1.70~\msol$ computed
    models. From left to right, $\Omega$ represents the rotational velocity
    in $\kms$;
    $\teff$ the effective temperature (on a logarithmic scale); $L/\lsol$ the
    luminosity in solar luminosities (on a logarithmic scale); $R/\rsol$ the stellar radius
    in solar radii; $g$ the surface gravity in cgs (on a logarithmic scale);
    the age in Myr; $\nu(\Pi_0)$ the frequency of
    the fundamental radial mode (in $\muHz$) and finally, $\Pi_1/\Pi_0$ represents the
    ratio between periods of the first overtone and the fundamental radial mode.
    Variables indexed with a $d$ represent the same quantities obtained when including
    near-degeneracy effects.}
    \begin{tabular}{ccccccccccc}
    \hline\hline
     & 
$\Omega$ & $\teff$ & $L/L_{\odot}$ & $R/\rsol$ & $g$ & Age & $\nu(\Pi_0)$ & $\Pi_0/\Pi_1$ & $\nu(\Pi_0^d)$ & $(\Pi_0/\Pi_1)^d$
 \\
    \hline
\par
m$_1$ & 50 & 3.853 & 1.045 & 2.184 & 3.989 & 1200.0 & 142.553 & 0.772 & 142.504 & 0.772
 \\
\par
m$_2$ & 100 & 3.851 & 1.042 & 2.202 & 3.982 & 1192.5 & 140.602 & 0.776 & 139.988 & 0.773
 \\
\par
m$_3$ & 150 & 3.849 & 1.033 & 2.192 & 3.986 & 1144.2 & 141.355 & 0.782 & 139.176 & 0.760
 \\
\par
m$_4$ & 200 & 3.847 & 1.017 & 2.181 & 3.990 & 1039.0 & 141.711 & 0.792 & 141.711 & 0.757
 \\
\par
m$_5$ & 250 & 3.854 & 0.991 & 2.046 & 4.045 & 830.0 & 156.566 & 0.798 & 147.819 & 0.722
 \\
\par
m$_6$ & 50 & 3.859 & 1.038 & 2.112 & 4.018 & 1132.0 & 150.315 & 0.773 & 150.166 & 0.772
 \\
\par
m$_7$ & 100 & 3.858 & 1.032 & 2.101 & 4.023 & 1094.9 & 151.447 & 0.776 & 150.303 & 0.770
 \\
\par
m$_8$ & 150 & 3.858 & 1.020 & 2.079 & 4.032 & 1027.5 & 153.719 & 0.782 & 150.688 & 0.767
 \\
\par
m$_9$ & 200 & 3.850 & 1.007 & 2.120 & 4.015 & 959.0 & 148.333 & 0.794 & 141.738 & 0.728
 \\
\par
m$_{10}$ & 250 & 3.859 & 0.981 & 1.976 & 4.076 & 741.0 & 165.481 & 0.797 & 156.385 & 0.753
 \\
\par
m$_{11}$ & 50 & 3.867 & 1.026 & 2.007 & 4.062 & 1021.0 & 162.571 & 0.773 & 162.616 & 0.773
 \\
\par
m$_{12}$ & 100 & 3.865 & 1.021 & 2.013 & 4.060 & 999.0 & 161.760 & 0.776 & 162.960 & 0.785
 \\
\par
m$_{13}$ & 150 & 3.866 & 1.006 & 1.972 & 4.078 & 898.3 & 166.858 & 0.782 & 170.549 & 0.799
 \\
\par
m$_{14}$ & 200 & 3.859 & 0.993 & 2.001 & 4.065 & 829.0 & 162.627 & 0.792 & 155.581 & 0.758
 \\
\par
m$_{15}$ & 250 & 3.864 & 0.970 & 1.906 & 4.107 & 634.0 & 175.117 & 0.797 & 165.244 & 0.752
 \\
\par
m$_{16}$ & 50 & 3.874 & 1.013 & 1.910 & 4.106 & 899.4 & 175.432 & 0.773 & 175.445 & 0.773
 \\
\par
m$_{17}$ & 100 & 3.875 & 1.002 & 1.879 & 4.119 & 823.0 & 179.763 & 0.776 & 179.988 & 0.784
 \\
\par
m$_{18}$ & 150 & 3.873 & 0.990 & 1.872 & 4.123 & 755.7 & 180.692 & 0.782 & 182.011 & 0.805
 \\
\par
m$_{19}$ & 200 & 3.867 & 0.980 & 1.903 & 4.108 & 699.0 & 175.909 & 0.791 & 182.864 & 0.822
 \\
\par
m$_{20}$ & 250 & 3.867 & 0.955 & 1.848 & 4.134 & 509.0 & 183.512 & 0.798 & 190.824 & 0.885
 \\
    \hline
    \end{tabular}
    \label{tab:altairmodels_m170}
\end{table}