Table 3
Dispersion ratio (Eq. (9)) of the inversions for rotational splittings computed with perturbed stellar models of KIC 7341231.
| ℓ | 1 | 1, 2 | 1, 2 | 1, 2 | 1 ,2 |
| ν [μHz] | 285 480 | 200 530 | 350 450 | ||
| ⟨ σi ⟩ [μHz] | 93 | 27 | 80 | 99 | 58 |
|
|
|||||
 (solid body) |
159 | 297 | 165 | 159 | 437 |
| (step) |
6.75 | 3.88 | 3.30 | 1.66 | 14.0 |
| (smooth) |
6.96 | 6.14 | 3.78 | 2.59 | 19.2 |
Notes. Frequency range for the first three columns is 285 μHz ≤ ν ≤ 480 μHz (22 modes). The first column includes only ℓ = 1 modes and the rest ℓ = 1,2 modes. In the third column, we reduced the uncertainty in the splittings to the equivalent of three years of observations. In the last two columns, we increased the frequency range to 200 μHz ≤ ν ≤ 530 μHz (26 modes) and decreased the frequency range to 350 μHz ≤ ν ≤ 450 μHz (13 modes) respectively, changing the uncertainties.
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