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Table 8

Stars with outlying radial velocities, which are candidate large-amplitude binaries or runaway stars.

Star Spectral type v1± s.d. (v1) | v1/σ v2± s.d. (v2) | v2/σ
[km s-1] [km s-1] [km s-1] [km s-1]

097 O9 IIIn 209.0 ± 15.3 65.1 ± 22.4 4.0 214.7 ± 9.5 59.6 ± 19.1 3.6
159 O3.5 III(f) 370.1 ± 5.7 96.0 ± 17.4 5.8 377.8 ± 7.2 103.5 ± 18.0 6.3
195 B1 Ib Nwk 328.3 ± 12.2 54.2 ± 20.4 3.3 329.9 ± 4.3 55.6 ± 17.1 3.4
254 O2 III-If ... ... ... 190.3 ± 1.6 84.0 ± 16.6 5.1
383 O9.2 Ib 189.0 ± 10.1 85.1 ± 19.3 5.2 ... ... ...
401 B0.5 Ia 222.5 ± 7.5 51.6 ± 18.0 3.1 216.1 ± 7.1 58.2 ± 18.0 3.5
424 B0.7 Ib Nwk 192.2 ± 10.2 81.9 ± 19.3 5.0 199.9 ± 7.1 74.4 ± 18.0 4.5
426 O6.5 III(f) 213.6 ± 14.5 60.5 ± 21.9 3.7 220.7 ± 12.0 53.6 ± 20.4 3.2
428 O7.5 V((f)) 166.4 ± 5.8 107.7 ± 17.4 6.6 163.7 ± 8.1 110.6 ± 18.4 6.7

Notes. The adopted mean velocities ( and ) are those from the first entry of Table 7 (which exclude the above stars and candidate binaries). AAΩ 30 Dor 254 = VFTS 016, the runaway star reported by Evans et al. (2010).

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