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Table A.2

Nitrogen abundances of presumed-single O-type sources with no luminosity class identifier.

VFTS SpTa νesini ε N σ N n l log  gc b
kms-1 dex dex cgs

051 OBpe 412 8.33 < 3.44
125 Ope 274 7.53 < 4.04
131 O9.7 124 8.09 < 4.59
142 Op 72 7.36 < 4.22
208 O6(n)fp 238 8.49 < 3.61
373 O9.5n 382 7.91 < 3.83
393 O9.5(n) 196 7.43 < 3.55
405 O9.5:n 290 7.88 < 3.85
412 O9.7 50 7.55 < 4.08
444 O9.7 100 7.66 < 4.23
456 Onn 480 8.03 < 3.93
465 On 276 7.54 < 3.77
476 O((n)) 176 7.42 < 3.31
477 O((n)) 94 7.76 < 3.88
515 O8-9p 50 7.29 0.11 2 3.89
519 O3-4((f)) 130 8.28 < 3.66
528 O9.7(n) 130 7.72 < 4.14
529 O9.5(n)SB? 284 8.17 < 4.34
539 O9.5(n) 126 7.76 < 4.08
559 O9.7(n) 204 8.13 < 4.20
579 O9:((n))SB? 88 7.42 < 3.94
587 O9.7:SB? 74 7.09 < 4.31
594 O9.7 44 7.51 < 4.20
626 O5-6n(f)p 288 9.03 < 3.70

Poor quality fits

145 O8fp 124 6.88 0.31 2 3.57
177 O7n(f)p 310 8.08 0.10 1 3.66
360 O9.7 400 8.23 < 3.37
400 O9.7 284 8.35 < 4.30
446 Onn((f)) 252 7.89 < 3.48
451 O(n) 296 8.17 < 3.79
565 O9.5:SB? 300 8.18 < 4.32

Notes. Upper limits are indicated by < in the fifth column and the number of lines used for the measurement nl is given in the sixth column. Abundances have been estimated with fixed ξm = 10 kms-1 (see Sect. 3.4). Poor quality fits are shown in a separate segment.

(a)

Spectral types as given by Walborn et al. (2014);

(b)

log  gc (cgs) is the logarithmic surface gravity corrected for centrifugal force. An electronic form of the table is available at the CDS.

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