Table 4: Idem Table 2 for $M=1.76~{M}_{\odot}$ models.
$\Omega$ ${T}_{{\rm eff}}$ $L/L_{\odot }$ $R/{R}_{\odot }$ g Age $\nu (\Pi _0)$ $\Pi_0/\Pi_1$ $\nu(\Pi_0^d)$ $(\Pi_0/\Pi_1)^d$

m₄₁
50 3.851 1.121 2.410 3.918 1200 124.959 0.773 124.943 0.772

m₄₂
100 3.848 1.117 2.429 3.911 1192.5 123.249 0.776 122.984 0.771

m₄₃
150 3.849 1.107 2.394 3.924 1144.2 125.873 0.782 124.407 0.756

m₄₄
200 3.847 1.092 2.375 3.931 1039.0 126.768 0.793 131.618 0.874

m₄₅
250 3.854 1.062 2.224 3.988 830.0 139.769 0.803 144.078 0.903

m₄₆
50 3.859 1.113 2.306 3.957 1132.0 133.931 0.773 133.896 0.773

m₄₇
100 3.859 1.106 2.285 3.965 1094.9 135.737 0.777 135.124 0.773

m₄₈
150 3.860 1.094 2.238 3.983 1027.5 139.989 0.783 137.570 0.769

m₄₉
200 3.857 1.083 2.248 3.979 959.0 138.644 0.791 133.851 0.736

m₅₀
250 3.861 1.051 2.123 4.029 741.0 150.734 0.801 150.734 0.758

m₅₁
50 3.870 1.100 2.161 4.013 1021.0 148.028 0.773 147.652 0.771

m₅₂
100 3.868 1.095 2.165 4.012 999.0 147.557 0.777 146.313 0.770

m₅₃
150 3.870 1.078 2.096 4.040 898.3 154.935 0.783 151.293 0.764

m₅₄
200 3.865 1.066 2.123 4.029 829.0 151.476 0.792 145.163 0.759

m₅₅
250 3.868 1.039 2.024 4.070 634.0 162.494 0.801 152.321 0.750

m₅₆
50 3.879 1.085 2.031 4.067 899.4 162.756 0.773 162.782 0.773

m₅₇
100 3.881 1.073 1.988 4.086 823.0 168.121 0.777 168.527 0.783

m₅₈
150 3.880 1.060 1.968 4.095 755.7 170.675 0.783 172.777 0.808

m₅₉
200 3.875 1.051 1.995 4.083 699.0 166.886 0.791 159.662 0.756

m₆₀
250 3.873 1.021 1.944 4.105 509.0 172.969 0.802 161.557 0.749

**Table 4:** Idem Table 2 for $M=1.76~{M}_{\odot}$ models.
	$\Omega$	${T}_{{\rm eff}}$	$L/L_{\odot }$	$R/{R}_{\odot }$	g	Age	$\nu (\Pi _0)$	$\Pi_0/\Pi_1$	$\nu(\Pi_0^d)$	$(\Pi_0/\Pi_1)^d$
m₄₁	50	3.851	1.121	2.410	3.918	1200	124.959	0.773	124.943	0.772
m₄₂	100	3.848	1.117	2.429	3.911	1192.5	123.249	0.776	122.984	0.771
m₄₃	150	3.849	1.107	2.394	3.924	1144.2	125.873	0.782	124.407	0.756
m₄₄	200	3.847	1.092	2.375	3.931	1039.0	126.768	0.793	131.618	0.874
m₄₅	250	3.854	1.062	2.224	3.988	830.0	139.769	0.803	144.078	0.903
m₄₆	50	3.859	1.113	2.306	3.957	1132.0	133.931	0.773	133.896	0.773
m₄₇	100	3.859	1.106	2.285	3.965	1094.9	135.737	0.777	135.124	0.773
m₄₈	150	3.860	1.094	2.238	3.983	1027.5	139.989	0.783	137.570	0.769
m₄₉	200	3.857	1.083	2.248	3.979	959.0	138.644	0.791	133.851	0.736
m₅₀	250	3.861	1.051	2.123	4.029	741.0	150.734	0.801	150.734	0.758
m₅₁	50	3.870	1.100	2.161	4.013	1021.0	148.028	0.773	147.652	0.771
m₅₂	100	3.868	1.095	2.165	4.012	999.0	147.557	0.777	146.313	0.770
m₅₃	150	3.870	1.078	2.096	4.040	898.3	154.935	0.783	151.293	0.764
m₅₄	200	3.865	1.066	2.123	4.029	829.0	151.476	0.792	145.163	0.759
m₅₅	250	3.868	1.039	2.024	4.070	634.0	162.494	0.801	152.321	0.750
m₅₆	50	3.879	1.085	2.031	4.067	899.4	162.756	0.773	162.782	0.773
m₅₇	100	3.881	1.073	1.988	4.086	823.0	168.121	0.777	168.527	0.783
m₅₈	150	3.880	1.060	1.968	4.095	755.7	170.675	0.783	172.777	0.808
m₅₉	200	3.875	1.051	1.995	4.083	699.0	166.886	0.791	159.662	0.756
m₆₀	250	3.873	1.021	1.944	4.105	509.0	172.969	0.802	161.557	0.749

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