Table 1.
Frequencies of the low-radial-order (k), low-degree (ℓ = 1, 2) g-modes computed for the optimal seismic model of KIC 08626021 derived by Giammichele et al. (2018), which does not include neutrino cooling (ν0), and for the equivalent model including this effect (ν2).
ℓ | k | ν0 (μHz) | ν2 (μHz) | ν0 − ν2 (μHz) | |
---|---|---|---|---|---|
1 | 1 | 8068.0321 | 8110.3577 | −42.3256 | |
1 | 2 | 6067.6415 | 6034.7152 | +32.9263 | |
1 | 3 | * | 5073.2341 | 5007.8906 | +65.3435 |
1 | 4 | * | 4309.9149 | 4269.5782 | +40.3367 |
1 | 5 | * | 3681.8029 | 3656.3533 | +25.4496 |
1 | 6 | * | 3294.3693 | 3246.8780 | +47.4913 |
1 | 7 | 2971.7185 | 2935.9436 | +35.7749 | |
1 | 8 | 2616.2037 | 2599.0472 | +17.1565 | |
1 | 9 | 2420.5893 | 2380.5206 | +40.0687 | |
1 | 10 | 2221.6371 | 2194.8451 | +26.7920 | |
2 | 2 | 9825.0553 | 9842.7756 | −17.7203 | |
2 | 3 | 8088.3782 | 8063.0609 | +25.3173 | |
2 | 4 | * | 6981.2613 | 6909.0377 | +72.2236 |
2 | 5 | 6110.7566 | 6081.0542 | +29.7024 | |
2 | 6 | 5399.5510 | 5370.1025 | +29.4485 | |
2 | 7 | 4859.1436 | 4774.7813 | +84.3623 | |
2 | 8 | * | 4398.3723 | 4371.7608 | +26.6115 |
2 | 9 | 3994.3952 | 3965.6973 | +28.6979 | |
2 | 10 | * | 3677.9937 | 3604.7042 | +73.2895 |
2 | 11 | 3406.5703 | 3386.6587 | +19.9116 | |
2 | 12 | 3138.9597 | 3114.3881 | +24.5716 | |
2 | 13 | 2967.7865 | 2913.2948 | +54.4917 | |
2 | 14 | 2808.2635 | 2789.5232 | +18.7403 | |
2 | 15 | * | 2658.7774 | 2649.2922 | +9.4852 |
2 | 16 | 2531.8834 | 2489.6276 | +42.2558 | |
2 | 17 | 2424.0703 | 2391.7391 | +32.3312 | |
2 | 18 | 2266.5570 | 2254.9941 | +11.5629 | |
2 | 19 | 2166.4153 | 2127.2743 | +39.1410 | |
2 | 20 | 2083.2448 | 2056.7203 | +26.5245 |
Notes. The modes marked by an asterisk are those fitted to the observed frequencies that closely match ν0. The last column lists the frequency differences for each mode, between the two models.
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