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Table 4

Stars with uncertain stellar parameters that are excluded from the discussion.

Star Spectral type src. log L/L Teff T log (/ ν ν Y n log Q0 M/M Γe νsini src. M V R V E(BV) E(VKs)
VFTS [kK] [kK] [M yr-1] [km s-1] [km s-1] [ph s-1] [km s-1] [mag]

063 O5 III(n)(fc)+ sec 1 5.76 42.2 42.3 –5.7 2910 0.25 ne 49.49 65 0.24 –5.7 4.56 0.321 1.27
094 O3.5 Inf*p + sec 1 5.98 42.2 42.3 –5.0 2690 0.325 e 49.71 79 0.31 –6.3 4.39 0.43 1.641
145 O8fp 1 5.87 39.8 39.9 –5.3 2470 0.4 e 49.55 65 0.28 93 i –6.2 3.92 0.511 1.748
147 WN6(h) 2 5.83 39.8 42.5 –4.5 1100 2030 0.7 e 49.61 43 0.31 < 200 iii
151 O6.5 II(f)p 1 6.03 42.2 42.3 –5.4 2550 0.4 e 49.77 79 0.33 89 i –6.4 2.09 0.423 0.802
208 O6(n)fp 1 5.64 37.6 37.7 –5.3 2530 0.325 e 49.25 53 0.21 271 i –5.8 3.02 0.649 1.731
402 WN7(h) + OB 2 5.92 39.8 46.4 –3.6 1800 1770 0.85 e 49.69 40 0.37 < 200 iii –6.7 0.85 0.575 0.495
406 O6 Vnn 1 5.48 37.6 37.7 –5.4 2600 0.325 e 49.09 44 0.18 356 i –5.4 3.67 0.329 1.058
440 O6-6.5 II(f) 1 5.88 39.8 39.9 –5.4 2690 0.25 e 49.56 76 0.27 94 i –6.2 4.06 0.34 1.205
445 O3-4 V:((fc)): + O4-7 V:((fc)): 1 5.78 44.7 44.9 –5.8 3070 0.25 ne 49.56 67 0.24 –5.6 4.39 0.422 1.607
468 O2 V((f*)) + OB 1 6.0 44.7 44.9 –5.5 2960 0.25 e 49.79 89 0.31 80 ii –6.1 6.22 0.361 1.928
509 WN5(h) + early O 2 6.43 42.2 42.3 –4.1 2200 1840 0.775 e 50.17 94 0.54 < 200 iii –7.4 5.37 0.295 1.364
527 O6.5 Iafc + O6 Iaf 1 6.29 34.0 34.9 –5.5 1200 0.25 e 49.99 –7.6 2.96 0.359 1.293
538 ON9 Ia: + O7.5: I:(f): 1 5.64 37.6 37.7 –5.5 2640 0.25 e 49.24 57 0.21 –5.8 4.49 0.289 1.124
562 O4V 9 6.05 42.2 42.3 –5.3 2780 0.25 e 49.79 94 0.32 –6.4 3.91 0.411 1.401
1014 O3 V + mid/late O 5, 6 6.22 44.7 44.9 –5.5 2870 0.25 ne 50.00 119 0.38 –6.7 6.52 0.366 2.044
1026 O3 III(f*) + mid/late O 5, 6 5.83 42.2 42.3 –5.5 2880 0.25 e 49.57 71 0.25 –5.9 4.74 0.403 1.653
1028 O3 III(f*) or O4-5V 5, 6, 10 6.09 47.3 47.7 –5.7 3100 0.25 e 49.91 99 0.33 –6.2 4.54 0.336 1.322

Notes. Sources: (1)Walborn et al. (2014); (2)Evans et al. (2011); (3)Crowther & Smith (1997); (4)Crowther & Walborn (2011); (5)Massey & Hunter (1998); (6)Hénault-Brunet et al. (2012); (7)Crowther & Dessart (1998); (8)Foellmi et al. (2003); (9)Melnick (1985); (10)Walborn & Blades (1997). Sources for νsini: (i) Ramírez-Agudelo et al. (2013); (ii) Sabín-Sanjulián et al. (2014); (iii) conservative upper limits from this work.

(†)

Y is the helium mass fraction;

(‡)

measured ν;

(▴)

calculated ν using Lamers et al. (1995) with Eq. (6), nitrogen abundance: n for normal, ne for between normal and enhanced, and e for enhanced;

(◆)

using the mass-luminosity relation chemical homogeneity by Gräfener et al. (2011).

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