Table 6
Probability tests to investigate the rotational velocities of the candidate runaway stars compared to those for the full (unevolved) B-type sample from Dufton et al. (2013).
| Test (from 104 repeats of 106 runs) | n | P |
|
|
||
| 4 × vesini ≤ 65 & 4 × vesini ≥ 345 kms-1 | 10 ± 3 | 0.0010 |
| 3 × vesini ≤ 40 & 4 × vesini ≥ 345 kms-1 | 6 ± 2 | 0.0006 |
| 4 × ve ≤ 100 & 4 × ve ≥ 340 kms-1 | 395 ± 20 | 0.0395 |
| 3 × ve ≤ 60 & 4 × ve ≥ 340 kms-1 | 181 ± 13 | 0.0181 |
Notes.“n”: number of Monte Carlo runs (from 106 sets) for which the simulated rotational velocities are consistent with those of the candidate runaways (and translated into a fractional probability, P, in the final column); the quoted uncertainties are the standard deviations from 104 repeat runs.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.