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Table 11.

Estimated component masses based on the mass function and primary’s spectral types and a range of orbital inclinations.

Object Spectral type P f(M) M1 M2 i
d  M  M  M degrees
Pre-mass transfer systems

HD 164 438 O9.2 IV 10.2 0.0198 15–20 1.8−4.6 30−90
HDE 229 234 O9 III 3.5 0.0450 18–23 3.1−7 30−70
Cyg OB2-41 O9.7 III(n) 29.4 0.2080 15–23 4.3−10 35−90
ALS 15 148 O6.5 V 3.1 0.0074 24–27 1.7−2.1 60−90
Cyg OB2-1 O8 IV(n)((f)) 4.9 0.1640 18–21 4.3−6 60−90
Cyg OB2-20 O9.7 IV 25.1 0.1640 15–18 3.9−9 35−90
Cyg OB2-15 O8 III 14.7 0.0950 20–25 3.8−11 25−90
Cyg OB2-11 O5.5 Ifc 72.5 0.0780 35–50 7−19 20−70
V747 Cep O5.5 V(n)((f)) 5.5 0.4360 27–30 8−11 60−90
HD 37 737 O9.5 II-III(n) 7.8 0.2200 18–25 5−7 60−90
HD 46 573 O7 V((f))z 10.7 0.0007 21–23 0.8−1.5 30−60
HD 52 533 A O8.5 IVn 22.0 1.0200 18–21 9−12 60−90

Ongoing mass-transfer systems

BD +36 4063 ON9.7 Ib 4.8 2.06 15–23 11−18 60−90
HD 16 429 AaAb O9.2 III 3.0 0.76 18–23 8−11 60−90

Collapsed companions

V479 Sct ON6 V((f))z 3.9 0.0028 24–27 1.4−12 10−60
Cyg X-1 O9.7 Iabp var 5.6 0.3410 20–40 6−16 35−60
HD 12 323 ON9.2 V 1.9 0.0053 15–18 1.4−1.6 60−90
HD 15 137 O9 II-IIIn 55.4 0.0082 15–20 1.5−9 10−60
HD 14 633 AaAb ON8.5 V 15.4 0.0041 18–20 1.3−9 10−60

Colliding wind binary or with compact companion

Cyg OB2-A11 O7 Ib(f) 15.4 0.0199 25–40 2.5−7 30−60

Notes. The mass function for each system is from the calculated orbit (see Table 10).

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