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Table 2.
The six stars with single retrograde period spacing patterns, which we suspect correspond to Yanai modes.
| KIC | v sin i (km s−1) | fdom (d−1) | Pmin (days) | Pmax (days) |
|---|---|---|---|---|
| 4757184 | 36(3) | 1.26725(2) | 0.64993(4) | 1.00612(7) |
| 5350598 | 28(2) | 2.158490(4) | 0.58249(2) | 1.36381(8) |
| 6185513 | 83(6) | 2.245965(7) | 0.50812(2) | 1.3940(1) |
| 6425437 | 50(3) | 0.89681(1) | 0.69305(6) | 1.2640(2) |
| 7867348 | 17(1) | 1.16998(1) | 1.14962(2) | 1.8273(2) |
| 11668783 | 34(3) | 0.627995(7) | 1.12644(4) | 1.65470(8) |
Notes. The listed parameters include the spectroscopic rotation velocity, the dominant pulsation frequency, and the minimum and maximum pulsation periods for the pulsations in the detected period spacing patterns.
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