Table 2.
Results of fitting asymptotic mode frequencies (including magnetic effects in a non-perturbative way) to the observed frequencies of the red giants in our sample.
| KIC Id | ΔΠ1 | δω0/2π | aasym | σB | ⟨Br2⟩0.5 | B0 |
|---|---|---|---|---|---|---|
| (s) | (μHz) | – | ( × 10−3 R★) | kG | MG | |
| KIC3326392 | ![]() |
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/
|
215 ± 7 | 5.1 |
| KIC5700274 | ![]() |
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179 ± 11 | 1.4 |
| KIC7458743 | ![]() |
![]() |
![]() |
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111 ± 4 | 0.8 |
| KIC9227589 | ![]() |
![]() |
![]() |
![]() |
681 ± 20 | 5.5 |
| KIC9697268 | ![]() |
![]() |
![]() |
![]() |
331 ± 36 | 3.3 |
| KIC10613561 | ![]() |
![]() |
![]() |
/
|
377 ± 39 | 1.4 |
| KIC10976412 | ![]() |
![]() |
![]() |
![]() |
114 ± 7 | 0.8 |
| KIC11408970 | ![]() |
![]() |
![]() |
/
|
333 ± 26 | 1.9 |
Notes. For KIC 3326392, KIC 10613561, and KIC 11408970, the distribution for σB is bimodal and the possible solutions are given. The last two columns give the average magnetic field strengths in the core ⟨Br2⟩0.5 measured using a stellar model, and the field strength B0 at the center for the median model (in MG).
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