Table A.1.
Frequencies of low-radial order (k) and low-degree (ℓ = 1 and 2) g-modes computed for the three identical models using various orders of correction for the luminosity profile.
ℓ | k | ν0 | ν1 | ν0 − ν1 | ν2 | ν1 − ν2 |
---|---|---|---|---|---|---|
(μHz) | (μHz) | (μHz) | (μHz) | (μHz) | ||
1 | 1 | 8068.03 | 8115.92 | −47.89 | 8110.36 | +5.56 |
1 | 2 | 6067.64 | 6033.94 | +33.70 | 6034.72 | −0.78 |
1 | 3 | 5073.23 | 5004.11 | +69.12 | 5007.89 | −3.78 |
1 | 4 | 4309.91 | 4266.71 | +43.20 | 4269.58 | −2.87 |
1 | 5 | 3681.80 | 3654.91 | +26.89 | 3656.35 | −1.44 |
1 | 6 | 3294.37 | 3243.91 | +50.46 | 3246.88 | −2.97 |
1 | 7 | 2971.72 | 2932.88 | +38.84 | 2935.94 | −3.06 |
1 | 8 | 2616.20 | 2598.02 | +18.18 | 2599.05 | −1.03 |
1 | 9 | 2420.59 | 2377.83 | +42.76 | 2380.52 | −2.69 |
1 | 10 | 2221.64 | 2192.15 | +29.49 | 2194.85 | −2.70 |
2 | 2 | 9825.06 | 9846.53 | −21.47 | 9842.78 | +3.75 |
2 | 3 | 8088.38 | 8063.63 | +24.75 | 8063.06 | +0.57 |
2 | 4 | 6981.26 | 6905.46 | +75.80 | 6909.04 | −3.58 |
2 | 5 | 6110.76 | 6079.26 | +31.50 | 6081.05 | −1.79 |
2 | 6 | 5399.55 | 5368.83 | +30.72 | 5370.10 | −1.27 |
2 | 7 | 4859.14 | 4769.59 | +89.55 | 4774.78 | −5.19 |
2 | 8 | 4398.37 | 4369.51 | +28.86 | 4371.76 | −2.25 |
2 | 9 | 3994.40 | 3964.17 | +30.23 | 3965.70 | −1.53 |
2 | 10 | 3677.99 | 3599.78 | +78.21 | 3604.70 | −4.92 |
2 | 11 | 3406.57 | 3384.34 | +22.23 | 3386.66 | −2.32 |
2 | 12 | 3138.96 | 3113.23 | +25.73 | 3114.39 | −1.16 |
2 | 13 | 2967.79 | 2909.93 | +57.86 | 2913.29 | −3.36 |
2 | 14 | 2808.26 | 2787.27 | +20.99 | 2789.52 | −2.25 |
2 | 15 | 2658.78 | 2648.59 | +10.19 | 2649.29 | −0.70 |
2 | 16 | 2531.88 | 2487.92 | +43.96 | 2489.63 | −1.71 |
2 | 17 | 2424.07 | 2387.97 | +36.10 | 2391.74 | −3.77 |
2 | 18 | 2266.56 | 2254.08 | +12.48 | 2254.99 | −0.91 |
2 | 19 | 2166.42 | 2125.98 | +40.44 | 2127.27 | −1.29 |
2 | 20 | 2083.24 | 2053.04 | +30.20 | 2056.72 | −3.68 |
Notes. The zeroth-order frequencies (ν0) correspond to the model assuming Lr ∝ Mr (model from Giammichele et al. 2018). The first-order frequencies (ν1) are determined with the model constructed from the interpolation of kν in the grid of “canonical” evolutionary models. The second-order frequencies (ν2) are from the model with the luminosity profile corrected for the particular chemical stratification of the model considered. Absolute differences in mode frequencies between the zeroth- and first-order, and between the first- and second-order are also given.
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