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Table E.2

113 O-type stars in the sample with double-line spectroscopic features, separated by luminosity class (I+II, III, and IV+V) and sorted by spectral type.

Name SpT LC B E(4405–5495) LC
(mag) comp.
HD 93162 O2.5 I f*/WN6 8.5 0.695 OB
LS III +4611 O3.5 I f* 12.5 1.726 O3.5If*
HD 228 766 O4 I f* 9.8 0.884 O8:II:
HDE 229196 O6 II (f) 9.4 1.158
HD 153919 O6 Ia fcp 6.8 0.499
HD 150958 O6.5 Ia (n)f 7.9 0.613
HD 152248 O7 Iab f 6.3 0.403 O7Ib(f)
HD 101205 O7 II: (n) 6.6 0.322
HD 57060 O7 Ia fp var 4.8 0.131
HD 166734 O7.5 Iab f 9.5 1.284
HD 167971 O8 Ia f(n) 8.9 0.986 O4/5
HD 149404 O8.5 Iab (f)p 5.9 0.621
HD 57061 AaAb O9 II 4.8 0.103
HD 323110 ON9 Ia 10.9 1.474
HD 1337 O9.2 II 6 0.140 O8V((f))
HD 35921 O9.5 II 7.3 0.425 O9III
HD 69106 O9.7 II n 7 0.214
HD 93206 O9.7 Ib n 7 0.342

HD 17505 O6.5+O8 III+V n(f)+... 7.7 0.636
HD 150136 O3.5-4 III (f*) 6.1 0.443 O6IV
HD 191201 O9.5+O9.7 III+III...+... 7.8 0.401 B0IV
HD 124314 O6+O9.2 IV+IV (n)((f))+(n) 7.5 0.457
HDE 319718 A O3.5 III (f*) 12.8 1.814
HD 15558 O4.5 III (f) 8.4 0.747
HD 93403 O5.5 III (fc) var 7.5 0.503
HD 93130 O6.5 III (f) 8.4 0.501
HD 167771 O7 III ((f)) 6.6 0.360 O8III
HD 115455 O8 III ((f)) 8.2 0.472
HDE 319702 O8 III 11 1.206
HD 47129 O8 ... fp var 6.1 0.331
HD 96670 O8.5 ... (n)fp var 7.9 0.444
HD 151003 O8.5 III 7.6 0.436
HD 153426 O8.5 III 7.6 0.392
HD 19820 O8.5 III (n)((f)) 7.6 0.763
HD 114886 O9 III 7.5 0.376 O9.5III
HD 16429 O9 II-III (n) Nwk 8.5 0.842
HD 37043 O9 III var 2.6 0.042
HD 93249 A O9 III 8.5 0.382
HD 15137 O9.5 II-III n 7.9 0.283
HD 167263 O9.5 III 6.1 0.268
HD 152219 O9.5 III (n) 7.8 0.416
HD 96264 O9.5 III 7.5 0.203
HD 156292 O9.7 III 7.8 0.502 B
HD 155775 O9.7 III (n) 6.7 0.243
HD 46106 O9.7 III (n) 8.1 0.392
HD 37468 AB O9.7 III 4.4 0.032
HD 117856 O9.7 II-III 7.6 0.433

HD 93205 O3.5 V ((f)) 7.8 0.351 O8V
LS III +4612 O4.5 IV (f) 11.4 1.323
HD 242908 O4.5 V (n)((fc))z 9.3 0.561
BD +45 3216 A O5 V ((f))z 10 0.685
HD 48099 O5.5 V ((f))z 6.3 0.243 O9V
V747 CEP O5.5 V (n)((f)) 11.4 1.641
ALS 12688 O5.5 V (n)((fc)) 11.3 0.860 B
BD -16 4826 O5.5 V ((f))z 10.6 1.032
HD 64315 O5.5 V 10.1 0.507 O7V
HD 215835 O5.5 V ((f)) 8.9 0.614 O6V((f))
HD 101131 O5.5 V ((f)) 7.4 0.319 O8:V
MY CAM O5.5 V (n) 10 0.565 O6.5V(n)
HD 165052 O6 V z 7 0.392 O8Vz
HDE 228 854 O6 IV n var 9.5 0.921 O5Vnvar
HD 92206 A O6 V ((f))z 8.3 0.406
CPD -59 2641 O6 V ((fc)) 9.5 0.603
HD 92206 B O6 V ((f)) 9.3 0.428
HD 168075 O6.5 V ((f)) 9.2 0.752
HD 194649 AB O6.5 V ((f)) 10.6 1.260
HD 150135 O6.5 V ((f))z 7.5 0.447
HDE 228 759 O6.5 V (n)((f))z 10.1 1.002
HD 18326 O6.5 V ((f))z 8.3 0.636 O9/B0V:
HD 206267 O6.5 V ((f)) 6.2 0.504 O9/B0V
HD 101436 O6.5 V ((f)) 7.7 0.354
BD +60 497 O6.5 V ((f)) 9.4 0.835 O8/B0V
Herschel 36 O7: V 11 0.825
HD 175514 O7 V (n)((f))z 9.2 0.848 B
ALS 12320 O7 IV ((f)) 11.2 0.996
ALS 8272 O7 V ((f)) 11.8 0.788 B0III-V
HD 135240 O7 IV ((f)) 5.2 0.208 B
HD 54662 O7 V z var? 6.8 0.305
HD 165921 O7 V (n)z 7.5 0.411 B0:V:
HD 319703 A O7 V ((f)) 11.9 1.476 O9.5V
HD 213023 A O7.5 V z 9.9 1.071
HDE 229 202 O7.5 V (n)((f)) 10.4 1.188
HD 93161 A O7.5 V 8.6 O9V
BD -14 5014 O7.5 V (n)((f)) 11.1 0.921
HD 97166 O7.5 IV ((f)) 8 0.351 O9III:
V572 CAR O7.5 V (n) 8.9 0.431 B0V(n)
BD +66 1675 O7.5 V z 10.1 1.403
BD +55 2840 O7.5 V (n) 10.6 0.771
HD 161853 O8 V (n)z 8.1 0.496 B
HD 100213 O8 V (n) 8.4 0.340 B0V(n)
CPD -59 2635 O8 V (n) 9.5 0.534 O9.5V
HD 17520 O8 V 9.1 0.589
HD 123590 O8 V z 8.4 0.418
HD 92206 C O8 V (n)z 9.1 0.424 B0:V
CPD -59 2636 O8 V 10.1 0.637 O8V
HD 93343 O8 V 9.8 0.524
HD 168137 AaAb O8 V z 10 0.678
HD 57236 O8.5 V 8.9 0.475
CPD -41 7733 O9 IV 7.9 0.441
HD 193322 O9 IV (n) 6.8 0.381
HD 75759 O9 V 6.1 0.185 B0V
HD 152218 O9 IV 7.8 0.454 B0:V:
HD 152314 O9 IV 8.2 0.493
HD 152246 O9 IV 8.1 0.428
HD 209481 O9 IV (n) var 5.6 0.326 B1:V:
HD 158186 O9.2 V 7.1 0.291 B1:V
HD 37366 O9.5 IV 7.7 0.365
HD 204827 O9.5 IV 9.3 1.072
HD 115071 O9.5 III 8.2 0.489 B0Ib
HD 164816 O9.5 V 7.1 0.258 B0V
HD 37041 O9.5 IV p 5 0.200
HD 198846 O9.5 IV 7.2 0.183 O9.5IV
HD 125206 O9.7 IV n 8.5 0.487

Notes. No analysis available. It details name, approximate spectral classification (sometimes is known to be a compromise, as the case of HD 37468, an SB3 star Simón-Díaz et al. 2015b; Maíz Apellániz et al. 2018), B magnitude, reddening parameter E(4405–5495), and secondary component spectral classification in the unresolved spectrum. Everything listed in GOSC (Maíz Apellániz et al. 2013) and Maíz Apellániz & Barbá (2018).

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