Table 2: Table containing the main characteristics of $M=1.70~{M}_{\odot}$ computed models. From left to right, $\Omega$ represents the rotational velocity in $\rm{km}~\rm{s}^{-1}$ ; ${T}_{{\rm eff}}$ the effective temperature (on a logarithmic scale); $L/L_{\odot }$ the luminosity in solar luminosities (on a logarithmic scale); $R/{R}_{\odot }$ 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 $\mu\mbox{Hz}$ ) 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.
$\Omega$ ${T}_{{\rm eff}}$ $L/L_{\odot }$ $R/{R}_{\odot }$ g Age $\nu (\Pi _0)$ $\Pi_0/\Pi_1$ $\nu(\Pi_0^d)$ $(\Pi_0/\Pi_1)^d$

m₁
50 3.853 1.045 2.184 3.989 1200.0 142.553 0.772 142.504 0.772

m₂
100 3.851 1.042 2.202 3.982 1192.5 140.602 0.776 139.988 0.773

m₃
150 3.849 1.033 2.192 3.986 1144.2 141.355 0.782 139.176 0.760

m₄
200 3.847 1.017 2.181 3.990 1039.0 141.711 0.792 141.711 0.757

m₅
250 3.854 0.991 2.046 4.045 830.0 156.566 0.798 147.819 0.722

m₆
50 3.859 1.038 2.112 4.018 1132.0 150.315 0.773 150.166 0.772

m₇
100 3.858 1.032 2.101 4.023 1094.9 151.447 0.776 150.303 0.770

m₈
150 3.858 1.020 2.079 4.032 1027.5 153.719 0.782 150.688 0.767

m₉
200 3.850 1.007 2.120 4.015 959.0 148.333 0.794 141.738 0.728

m₁₀
250 3.859 0.981 1.976 4.076 741.0 165.481 0.797 156.385 0.753

m₁₁
50 3.867 1.026 2.007 4.062 1021.0 162.571 0.773 162.616 0.773

m₁₂
100 3.865 1.021 2.013 4.060 999.0 161.760 0.776 162.960 0.785

m₁₃
150 3.866 1.006 1.972 4.078 898.3 166.858 0.782 170.549 0.799

m₁₄
200 3.859 0.993 2.001 4.065 829.0 162.627 0.792 155.581 0.758

m₁₅
250 3.864 0.970 1.906 4.107 634.0 175.117 0.797 165.244 0.752

m₁₆
50 3.874 1.013 1.910 4.106 899.4 175.432 0.773 175.445 0.773

m₁₇
100 3.875 1.002 1.879 4.119 823.0 179.763 0.776 179.988 0.784

m₁₈
150 3.873 0.990 1.872 4.123 755.7 180.692 0.782 182.011 0.805

m₁₉
200 3.867 0.980 1.903 4.108 699.0 175.909 0.791 182.864 0.822

m₂₀
250 3.867 0.955 1.848 4.134 509.0 183.512 0.798 190.824 0.885

**Table 2:** Table containing the main characteristics of $M=1.70~{M}_{\odot}$ computed models. From left to right, $\Omega$ represents the rotational velocity in $\rm{km}~\rm{s}^{-1}$ ; ${T}_{{\rm eff}}$ the effective temperature (on a logarithmic scale); $L/L_{\odot }$ the luminosity in solar luminosities (on a logarithmic scale); $R/{R}_{\odot }$ 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 $\mu\mbox{Hz}$ ) 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.
	$\Omega$	${T}_{{\rm eff}}$	$L/L_{\odot }$	$R/{R}_{\odot }$	g	Age	$\nu (\Pi _0)$	$\Pi_0/\Pi_1$	$\nu(\Pi_0^d)$	$(\Pi_0/\Pi_1)^d$
m₁	50	3.853	1.045	2.184	3.989	1200.0	142.553	0.772	142.504	0.772
m₂	100	3.851	1.042	2.202	3.982	1192.5	140.602	0.776	139.988	0.773
m₃	150	3.849	1.033	2.192	3.986	1144.2	141.355	0.782	139.176	0.760
m₄	200	3.847	1.017	2.181	3.990	1039.0	141.711	0.792	141.711	0.757
m₅	250	3.854	0.991	2.046	4.045	830.0	156.566	0.798	147.819	0.722
m₆	50	3.859	1.038	2.112	4.018	1132.0	150.315	0.773	150.166	0.772
m₇	100	3.858	1.032	2.101	4.023	1094.9	151.447	0.776	150.303	0.770
m₈	150	3.858	1.020	2.079	4.032	1027.5	153.719	0.782	150.688	0.767
m₉	200	3.850	1.007	2.120	4.015	959.0	148.333	0.794	141.738	0.728
m₁₀	250	3.859	0.981	1.976	4.076	741.0	165.481	0.797	156.385	0.753
m₁₁	50	3.867	1.026	2.007	4.062	1021.0	162.571	0.773	162.616	0.773
m₁₂	100	3.865	1.021	2.013	4.060	999.0	161.760	0.776	162.960	0.785
m₁₃	150	3.866	1.006	1.972	4.078	898.3	166.858	0.782	170.549	0.799
m₁₄	200	3.859	0.993	2.001	4.065	829.0	162.627	0.792	155.581	0.758
m₁₅	250	3.864	0.970	1.906	4.107	634.0	175.117	0.797	165.244	0.752
m₁₆	50	3.874	1.013	1.910	4.106	899.4	175.432	0.773	175.445	0.773
m₁₇	100	3.875	1.002	1.879	4.119	823.0	179.763	0.776	179.988	0.784
m₁₈	150	3.873	0.990	1.872	4.123	755.7	180.692	0.782	182.011	0.805
m₁₉	200	3.867	0.980	1.903	4.108	699.0	175.909	0.791	182.864	0.822
m₂₀	250	3.867	0.955	1.848	4.134	509.0	183.512	0.798	190.824	0.885

Source LaTeX | All tables | In the text

	1 Introduction
	2 Fundamental parameters
	3 Modelling the star
	4 Comparison between theory and observations
	5 Conclusions
	References