Table 2.
Some statistics of interest for the cleaned slow- and fast-rotating samples (i.e. excluding three stars with V > 10 and/or d > 3 kpc from the initial sample, see text).
| v sin i |
< 200 km s−1 |
> 200 km s−1 |
|||||
|---|---|---|---|---|---|---|---|
| All | All | Runaways | |||||
| # | % | # | % | # | % | ||
| Total | 268 | 51 | 24 | 47 |
|||
| SB1 | 35 | 13 |
9 | 18 |
1 | 11 |
|
| SB2 | 89 | 33 |
4 | 8 |
0 | ... | |
| LPV/SB2? | 0 | ... | (2) | (4 ) |
0 | ... | |
| LS | 143 | 54 |
36 | 70 |
23 | 64 |
|
Notes. Percentages in the ‘all’ columns refer to total in each group (268 and 51, respectively), while these are computed with respect to the total number of fast-rotating stars per subgroup in the case of runaways (51, 9, and 38, respectively). See also the note about the relative percentage of LS and SB1 runaways for stars with v sin i below 200 km s−1 in Sect. 4.4.
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