J/A+A/564/A40 VFTS. O-type stellar content of 30 Dor (Walborn+, 2014)

J/A+A/564/A40/V//VFTS_7_/tablea1.dat BBB-rated spectral classifications and supporting data for 139 VFTS O-B0 stars (139 records)

VFTS
---		SpType
---		Mult
---		AltID
---		Com
---
017B0 V SB1l
035O9.5 IIIn SB2? VM2?
042O9.5 III((n)) SB1l SiIV weak, -4.7
047O9 V + O9.5 V SB2
049O9.7 V: + B SB2
051OBpe ST1-06
055O8.5 V + O9.5 IV SB2 VM2
056O6.5 V + O6.5 V SB2 ST1-07 H, He profiles triangular
058O8.5: V + B SB2 ST1-09
059O9.5 III: SBl ST1-10 SiIV very weak, -3.8
061ON8.5 III: + O9.7: V: SB2
063O5 III(n)(fc) + sec SB2 ST1-11
066O9.5 III(n) SBl SiIV very weak, -4.5
070O9.7 II SB? SiIV very weak
077O9.5: IIIn ST1-22 SiIV very weak, -3.4
080O9.7 II-III((n)) ST1-23 SiIV weak, -4.2
097B0 IV SB? ST1-31
102O9: Vnnne+ ST1-32 FeII emission; Dufton et al. (2011ApJ...743L..22D); runaway
104O9.7 II-III((n)) SiIV very weak
105O8: Vz + O9-B0 SB2 VM3 ST1-37
109O9.7 II:n ST1-38 HeII {lambda}4686 emission wings, "Onfp"? SiIV very weak
113O9.7 II or B0 IV ? SBs ST1-39 very sharp lines; HeII broad; SiIV very weak
114O8.5 IV + sec SB2 ST1-41
116O9.7: V: + B0: V: SB2 VM2? ST1-42
120O9.5 IV: SB2 ST1-43
125Ope SB2? ST1-47 or n with HeII emission; HeI {lambda}4713 double
128O9.5 III:((n)) ST1-49 SiIV weak, -3.3
131O9.7
141O9.5 II-III((n)) SB? T88-6 SiIV very weak, -4.3; Walborn et al. (1999AJ....118.1684W) B0.2 V
142Op ST1-58 composite: HeII/HeI {lambda}4541/{lambda}4471 implies O6.5, but {lambda}4541/{lambda}4387 & {lambda}4200/{lambda}4144 O8.5; false Vz
145O8fp SB1s T88-3 contaminated by Brey 73-1A; Walborn et al. (1999AJ....118.1684W) O7-8 II
148O9.7 II-III(n) SBl NC SiIV very weak
150O9.5 III SB2 T88-4 "Onfp"? SiIV very weak, -4.6; Walborn et al. (1999AJ....118.1684W) O9.5 V
151O6.5 II(f)p SBvs VM5 T88-2 composite: weak NIV & CIV emission, NV absorption; Walborn et al. (1999AJ....118.1684W), 3 components: O4 III(f)p, O8 III, B1-2:p(e)
153O9 III((n)) VM3 T88-5 SiIV weak, -5.0; Walborn et al. (1999AJ....118.1684W) O7 V(z!) N strong
163O8.5 IV "((n))" but profiles triangular & variable
173O9.7: II-III(n)p SBl ST1-73 "Onfp"; SiIV weak
174O8 V + B0: V: SB2 ST1-75
176O6 V:((f)) + O9.5: V: SB2 ST1-77
183B0 IV SB?
187O9 IV: + B0: V: SB2 ST1-81
188O9.7: III: SB? SiIV very weak, -4.0
192O9.7 II or B0 IV ? ST1-85 SiIV weak
201O9.7 V + sec SB2
205O9.7 II((n)) or B0 IV((n)) ? ST1-91 SiIV, CIII very weak
207O9.7 II((n)) ST1-92 SiIV, CIII very weak
217O4 V((fc)): + O5 V((fc)): SB2 ST1-98 X-ray source
226O9.7 III runaway; SiIV weak, -3.2
231O9.7 IV:(n) + sec SB2 ST1-103
241B0 IV SiIV weak
242B0 IV SB? runaway, SiIV weak
253O9.5 II SiIV very weak, -4.6; H strong
304O9.7 III VM2? SiIV weak; shallow WFC3 image appears extended, but deep symmetrical
310O9.7 V: contaminated by R135
313B0 IV SiIV weak
314O9.7 IV:(n) + sec: SB2
316O9.7 V: contaminated
318O((n))p SBl composite: He lines imply O9.5 III; H{delta} B2 V from strong wings and no SiIV, CIII; weak, narrow NIV emission, NV absorption present; -2.6
327O8.5 V(n) + sec SB2 P15
328O9.5 III(n) SB? SiIV weak, -3.3; runaway
329O9.7 II-III(n) SBl P19 SiIV weak
339O9.5 IV(n) P83 SiIV weak, -3.8
345O9.7 III(n) SBl P103 SiIV very weak, -4.1
346O9.7 III P113 SiIV very weak, -3.6
347B0 V P116 -2.8
350O8 V SB2 P124 circular nebula, Rubio et al. (1998)
352O4.5 V(n)((fc)):z: + O5.5 V(n)((fc)):z: SB2
360O9.7 P169 SiIV strong; no HeI {lambda}4713
370O9.7 III SB? P222 SiIV weak, -3.4; runaway
371O9.5 V(n) + sec SB2 P240
373O9.5n P246
389O9.5 IV Mk58(E)P304 SiIV weak, -5.1; Walborn et al. (2002AJ....124.1601W) O9.5 V; inadvertently "Mk58(w)" in Paper I
393O9.5(n) P324
400O9.7 P348
405O9.5:n
412O9.7
443O7: V(n): + O7: V(n): SB2 VM2 P615
444O9.7 SB?
445O3-4 V:((fc)): + O4-7 V:((fc)): SB2 P621 X-ray source
446Onn((f))
450O9.7 III: + O7:: SB2 Mk50 P643 I. Howarth et al., in prep.
451O(n) contaminated; bright circumstellar nebulosity
455O5: V:n SB1l P661 X-ray source
456Onn ((fc))?
460O7.5 V + O7.5 V SB2 P674
464O9.5: VM2 P702
465On P700
475O9.7 III SBl P722 SiIV weak, -4.5
476O((n))
477O((n)) contaminated? HeI {lambda}4713 Oe?
487O6.5: IV:((f)): + O6.5: IV:((f)): SB2 VM2
492O8 V + O9.5: V SB2 Mk21 P830
495O9.7 II-IIIn P9019 SiIV very weak
496B0 Vn SB? -3.8
497O3.5 V((f))z + OB R140d contaminated
500O6.5 IV((fc)) + O6.5 V((fc)) SB2 X-ray source
514O9.7 III SBl P9021 SiIV weak, -3.2
515O8-9p VM2 (subtract 513!) "Onfp"? variable? SiIV & CIII strong, HeII {lambda}4686 weak imply high luminosity
519O3-4 ((f)) + OB + WN SB1s R140c contaminated
522O6 II-Iab(fc) + O5.5 V((fc)): SB2
525B0 Ia SB Mk38 P930
527O6.5 Iafc + O6 Iaf SB2 R139 P952 Taylor et al. (2011); X-ray source
528O9.7(n) P956 "Onfp"? SiIV very weak
529O9.5(n) SB? P955
538ON9 Ia: + O7.5: I:(f): SB2 VM2 Mk22 P1024
539O9.5(n) P1012
540B0 V -3.8
543O9 IV + O9.7: V SB2 P1031
552O8.5 III: + B SB2
557On SB2
559O9.7(n) P1133
561O9:(n) SB1l P1145
563O9.7 III: + B0: V: SB2 VM2 P1154
565O9.5: SB?
570O9.5ne+ SB2 FeII emission
571O9.5 II-III(n) SB2? SiIV weak
579O9:((n)) SB? VM2 P1201 Knot 1; Walborn et al. (2002AJ....124.1601W) O9.5 V; X-ray source
583O8 V + O8.5 V SB2
587O9.7: SB?
588O9.5 SB1l "Onfp"? SiIV weak
594O9.7
607O9.7 III SB? SiIV weak, -3.6
622O9.7 III SB? SiIV weak
634O V VM2 P1473 z?
642O5 Vz: + O8 Vz: SB2
647O8: V:
652B2 Ip + O9 III: SB2 Mk5 P1552 I. Howarth et al., in prep.
661O6.5 V(n) + O9.7: V: SB2 P1594
703O7: V: + O8: V: SB2 P1828
711O9.7 III P1850 SiIV very weak, -4.2
728O9.7 II-III((n)) SBl P1966 SiIV weak
733O9.7p SBl P1988 "Onfp"; HeII wings; SiIV weak; NII {lambda}3995 too strong
771O9.7 III:(n) SB2 P2104
774O7.5 IVp + O8.5: V: SB2 SB3? He strong?
787O9.7 III SB P2157 SiIV weak, -3.5
806O5.5 V((fc)):z + O7 Vz: SB2 NC BI259
810O9.7 V + B1: V: SB2 P2242
859O9.5 IV + sec SB2
887O9.5 II-IIIn SB2 NC SiIV very weak, -4.4