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Table 5

Candidate runaway stars identified from the radial-velocity analysis of the VFTS B-type spectra.

VFTS Classification vr (vr) | vr/σ vesini r d
[kms-1] [kms-1] [kms-1] [] [pc]

242 B0 V-IV 216.0 ±3.6 55.6 ± 12.7 4.6 40 5.96 86.6
298 B1-2 V-IIIe+ 332.1 ±4.0 60.5 ± 12.8 5.0 431 ± 15 3.92 57.1
358 B0.5: V 164.7 ± 10.7 106.9 ± 16.2 8.8 345 ± 22 3.02 44.0
368 B1-3 V 229.6 ± 12.4 42.0 ± 17.4 3.4 380: 1.20 17.5
467 B1-2 Ve+ 322.3 ± 30.2 50.7 ± 32.6 4.2 355 ± 29 9.54 138.7
616 B0.5: V 227.4 ± 10.7 44.2 ± 16.2 3.6 40 1.26 18.3
625 B1.5 V 310.7 ±9.2 39.1 ± 15.3 3.2 64 ± 12 2.57 37.4
831 B5 Ia 210.4 ±6.2 61.2 ± 13.7 5.0 41 7.91 115.0
851 B2 III 229.4 ±0.3 42.2 ± 12.2 3.5 40 7.18 104.4

Notes. Estimates of vesini are from Dufton et al. (2013) except for VFTS 831, which is taken from McEvoy et al. (2014). Projected distances from the core of R136 are from Paper I.

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