Table 13
Estimates of the mean rotation rate in the g-mode cavity ⟨ Ωg ⟩, the mean rotation rate in the p-mode cavity ⟨ Ωp ⟩, and the ratio between these quantities obtained from the coefficients of the δν(ζ) relation (see Sect. 6.1) or from OLA inversions (see Sect. 6.2).
Star | ⟨ Ωg ⟩ /(2π) (nHz) | ⟨ Ωp ⟩ /(2π) (nHz) | ⟨ Ωp ⟩ / ⟨ Ωg ⟩ | |||||
|
||||||||
δν(ζ) | OLA | δν(ζ) | OLA | δν(ζ) | OLA | |||
|
||||||||
A (KIC 12508433) | 505 | 532 ± 79 | 227 | 213 ± 26 | 2.2 | 2.5 ± 0.7 | ||
B (KIC 8702606) | 619 | 629 ± 109 | 263 | 164 ± 17 | 2.4 | 3.8 ± 1.1 | ||
C (KIC 5689820) | 917 | 865 ± 35 | 109 | 125 ± 13 | 8.4 | 6.9 ± 1.0 | ||
D (KIC 8751420) | 1620 | 1540 ± 50 | 109 | 102 ± 24 | 14.8 | 15.1 ± 4.0 | ||
E (KIC 7799349) | 1323 | 1313 ± 26 | 86 | 122 ± 15 | 15.4 | 10.7 ± 1.5 | ||
F (KIC 9574283) | 1640 | 1556 ± 22 | 26 | 74 ± 28 | 64.1 | 21.0 ± 8.2 |
Notes. ⟨ Ωg ⟩ represents the average rotation rate in the g-mode cavity (innermost 1.5% to 2.5% of the star) and ⟨ Ωp ⟩ a weighted average of the rotation rate in the p-mode cavity, which can be regarded as an upper limit of the rotation rate in the convective envelope (see text).
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