Table 2
v sin i statistics for six star subsamples depicted in Fig. 8.
| Sample with v sin i < 150 km s−1 | Sample with v sin i > 150 km s−1 | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| LS | SB1 | LS | SB1 | |||||||||||
| Nall | NLS | % | (v sin i) | NSB1 | % | (v sin i) | Nall | NLS | % | (v sin i) | NSB1 | % | (v sin i) | |
| a) | 59 | 47 | 80 | 65 ± 19 | 12 | 20 | 80 ± 30 | 17 | 14 | 82 | 252 ± 65 | 3 | 18 | 197 ± 46 |
| b) | 103 | 85 | 82 | 73 ± 24 | 18 | 18 | 92 ± 30 | 21 | 18 | 86 | 241 ± 50 | 3 | 14 | 171 ± 9 |
| c) | 50 | 41 | 82 | 53 ± 38 | 9 | 18 | 83 ± 40 | 35 | 25 | 71 | 300 ± 82 | 10 | 29 | 223 ± 36 |
Notes. Extracted from the v sin i distribution associated with the six star subsamples depicted in Fig. 8 (LS and SB1 stars in a, b, and c panels), separated in two ranges of v sin i, comprising the low-velocity peak (v sin i < 150 km s−1) and the tail of fast rotators (v sin i > 150 km s−1). The columns labeled with (v sin i) quote the mean and standard deviation of the v sin i distribution within the indicated range.
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