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Table 2.

v sin i-estimates for primaries and secondaries in the SB2 sample denoted by subscripts 1 and 2, together with σ-estimates and the number of lines (n) used for these determinations.

VFTS Spectral types v sin i1 σ1 n1 v sin i2 σ2 n2

Evans (a) Primary (b) Secondary (b) (km s−1) (km s−1)
112 Early-B B0.5 V B1: V: 141 17 6 109 40 4
199 Early-B B2 V B2: V: 98 14 4 81 7 4
206 B3 III: B3 III-V 56 7 4
240 B1-2 V B1: V 141 16 2
248 B2: V B1.5 V 96 27 6
255 B2: V B2 V B2: V: 67 16 5 59 14 3
364 B2.5: V B2.5 V 96 8 5
383 B0.5: V B0.5 V 61 8 6
520 B1: V B1 V B1.5: V: 81 8 7
589 B0.5 V B0.5 V B1: V: < 40 < 40
637 B1-2 V+EarlyB B1.5 V 138 9 4
686 B0.7 III B0.7 III < 40
752 B2 V B1.5 V B1.5: V: 70 7 6 67 3 3
883 B0.5 V B0.5 V 96 16 3

Notes. Spectral types are also listed, where available. Spectral types from:

(a)

Evans et al. (2015), primaries only, and

(b)

present work.

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