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Table 3
Frequency of stars (f) from different subsamples that are spinning more rapidly than the specified limit.
| f(νesini) | |||
| Sample | >200 kms-1 | >250 kms-1 | >300 kms-1 |
|
|
|||
| Presumed-single | 0.193 ± 0.028 | 0.156 ± 0.024 | 0.104 ± 0.019 |
| Primaries | 0.175 ± 0.035 | 0.088 ± 0.026 | 0.026 ± 0.018 |
| Primaries (SB2) | 0.161 ± 0.065 | 0.032 ± 0.032 | 0.000 (<0.032) |
| Secondaries | 0.097 ± 0.065 | 0.032 ± 0.032 | 0.032 ± 0.032 |
| Low-ΔRV | 0.141 ± 0.035 | 0.082 ± 0.035 | 0.035 ± 0.024 |
| High-ΔRV | 0.276 ± 0.069 | 0.103 ± 0.069 | 0.000 (<0.034) |
Notes. 68% confidence intervals (approx. ±1 sigma error bars) were computed following binomial statistics (Sana et al. 2014).
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