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Table 3

Stellar and wind parameters derived for the O-type stars in four Cygnus OB associations.

Source SpT T eff log g log g true a R log(theo)b logc f v β vsini v mac M evol d M spec e M dyn f N/H
[kK] [R] [km s-1] [km s-1] [km s-1] [M] [M] [M] [× 10-4]

Cyg OB1

HD 193443P O 9III 31.2 5.35 ± 0.13 3.65 3.66 ~−6.8 105 38 1.0 ± 0.1 0.6 ± 0.3
HD 193443S O 9.5V 29.7 4.76 ± 0.23 3.75 3.76 100 27 0.4 ± 0.1 0.6 ± 0.3
HD 193514 O 7–7.5III(f) 34.5 5.65 ± 0.09 3.50 3.51 − 6.5 − 5.6 0.03 2190 1.5 90 27 2.0 ± 1.0
HD 193595 O 7V 35.5 5.11 ± 0.05 3.75 3.75 − 8.7 1.0 50 28 3.0 ± 1.5
HD 193682 O 5III(f) 39.4 5.50 ± 0.09 3.75 3.77 − 5.8 − 5.7 0.01 2650 1.0 150 73 6.0 ± 3.0
HD 194094 O 8III 29.9 5.45 ± 0.36 3.25 3.26 − 6.7 − 7.0 1.0 65 32 1.0 ± 0.5
HD 194280 O 9.7I 26.9 5.61 ± 0.36 3.10 3.11 <−6.5 92 41 0.1 ± 0.1
HD 228841 O 7 34.5 5.42 ± 0.37 3.50 3.62 ~−6.4 − 7.1 1.0 317 0 5.4 ± 2.7
HD 228989P O 8.5V 29.4 4.43 ± 0.14 3.50 3.56 145 3 7.0 ± 0.2 1.0 ± 0.5
HD 228989S O 9.7V 27.8 4.28 ± 0.15 3.75 3.78 120 3 6.1 ± 0.2 3.0 ± 1.5
HD 229234 O 9III + ... 32.0 5.09 ± 0.20 3.60 3.61 ~−6.8 − 6.5 1.0 85 38 0.6 ± 0.3

Cyg OB3

HD 190864 O 6.5III(f) 38.0 5.35 ± 0.14 3.75 3.76 − 6.3 − 6.4 0.06 2250 1.0 80 43 5.0 ± 3.0
HD 227018 O 6.5 37.3 5.50 ± 0.18 4.00 4.00 − 6.9 1.0 70 35 1.0 ± 0.5
HD 227245 O 7III 36.0 5.18 ± 0.14 3.75 3.75 ~−6.4 − 6.7 1.0 65 19 3.0 ± 0.5
HD 227757 O 9V 32.0 4.73 ± 0.13 3.75 3.75 − 8.2 1.0 45 3 0.6 ± 0.3

Cyg OB8

HD 191423 ON 9IIIn 30.6 5.42 ± 0.28 3.50 3.67 ~−6.8 − 6.4 0.01 600 0.9 410 0 5.4 ± 2.5
HD 191978 O 8III 33.2 5.35 ± 0.23 3.75 3.75 − 6.7 − 8.7 1.0 1600 40 32 3.0 ± 1.5
HD 193117 O 9III 30.1 5.36 ± 0.11 3.30 3.31 ~−6.8 − 6.3 1.0 80 28 0.6 ± 0.3

Cyg OB9

HD 194334 O 7–7.5III(f) 33.9 5.19 ± 0.07 3.50 3.51 ~−6.5 − 6.2 1.0 62 32 3.0 ± 1.5
HD 194649P O 6III(f) 38.0 5.14 ± 0.15 3.75 3.75 − 6.1 60 67 4.9 ± 0.4 3.0 ± 1.3
HD 194649S O 8V 33.0 4.36 ± 0.27 3.75 3.76 60 27 1.9 ± 0.1 1.0 ± 0.5
HD 195213 O 7III(f) 35.3 5.19 ± 0.22 3.50 3.51 ~−6.4 − 6.0 1.0 85 28 6.0 ± 3.0

Notes.

(a)

gtrue: gravity corrected from the contribution of the centrifugal force i.e. gtrue = g + (vsini)2/R;

(b)

log(theo): theoretical mass-loss rate estimated by Muijres et al. (2012) for a given spectral classification;

(c)

log(Hα): mass-loss rate (where the correction of the clumping is not applied) computed from the Hα line;

(d)

Mevol: mass estimated from the HR diagram;

(e)

Mspec: mass computed from M = gR2/G;

(f)

Mdyn: minimum mass of a binary component (M3 sini).

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