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Table 2
Classification of the main-sequence stars in our sample according to the type of variability observed in the Kepler light curves.
| SpT | Main sequence | With rotation | No. period | Ecl. binaries | Other | Pulsators | Unclear |
|---|---|---|---|---|---|---|---|
| (MS) stars | period | binaries | |||||
| All | 102 | 74 | 2 | 10 | 5 | 3 | 3 |
| A | 3 | 2 | 0 | 0 | 0 | 1 | 0 |
| F | 37 | 24 | 2 | 5 | 2 | 1 | 1 |
| G | 26 | 19 | 0 | 1 | 0 | 1 | 1 |
| K | 28 | 21 | 0 | 4 | 3 | 0 | 0 |
| M | 8 | 8 | 0 | 0 | 0 | 0 | 1 |
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