Table 14
Results from the initial pattern fitting of the observed period series.
| frot (d-1) | dPasym (s) | Mode ID (ℓ,m) | |
|
|
|||
| KIC 3459297 |
|
|
(1, + 1), (2, + 2) |
| KIC 6352430 A |
|
|
(1, + 1) |
| KIC 4930889 (A?) |
|
|
(1, + 1), (2,−2) |
| KIC 9020774 |
|
|
(1, + 1) |
| KIC 11971405 |
|
|
(1, + 1), (2, + 2) |
Notes. For comparison, we recall the rotation frequencies derived – using different methods – for the two slower rotator stars that are used for comparison in this paper: KIC 10526294 has a radius averaged rotation frequency of around 0.005 d-1 (Triana et al. 2015) and KIC 7760680 rotates at 0.48 d-1 (Moravveji et al. 2016).
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