Table 3
Results for the 20 BWE stars discussed here for all the OBs.
| ID | OB (Sp) | Hα | FWZI | EW(Li) | RV | vsin(i) | X | RV | MEMBERSHIP | ||
| Profile type | (Å) | (mÅ) | (km s-1) | (km s-1) | Li | Hα | TOT | ||||
|
|
|||||||||||
| 10 151 | OBA-2 (62) | (I) | − | − | −9.45 ± 3.27 | 17.7 ± 1.7 | N | Y | N | N | N |
| 10 151 | OBB-2 (51) | (I) | − | − | −10.91 ± 2.91 | <17 | |||||
| 10 151 | OBC-2 (51) | (I) | − | − | −9.68 ± 2.56 | <17 | |||||
|
|
|||||||||||
| 11 447 | OBA (74) | IV-B | 2.8−3.9 | − | −51.48 ± 3.43 | 21.1 ± 2.1 | N | N | N (V?) | Y | Y |
| 11 447 | OBB (74) | IV-B | − | −38.38 ± 3.50 | 19.4 ± 2.0 | ||||||
| 11 447 | OBC (74) | IV-B | − | − | − | ||||||
|
|
|||||||||||
| 11 532 | OBA (75) | (III-B) | − | − | 10.69 ± 2.46 | 20.3 ± 1.4 | N | B? | N | Y SKY | ? |
| 11 532 | OBB (76) | (I) | − | − | − | − | |||||
| 11 532 | OBC (76) | (I) | − | − | 26.21 ± 2.61 | <17 | |||||
|
|
|||||||||||
| 11 598 | OBA (64) | IV-B | 4.1−4.2 | − | −71.22 ± 3.77 | <17 | − | N | N (V?) | Y | Y |
| 11 598 | OBB (71) | IV-B | − | −58.63 ± 5.15 | <17 | − | |||||
| 11 598 | OBC (80) | IV-B | − | −59.95 ± 4.67 | <17 | − | |||||
|
|
|||||||||||
| 11 751 | OBA (88) | early | − | − | − | N | − | N | early | ? | |
| 11 751 | OBA-2 (82) | early | − | − | − | ||||||
| 11 751 | OBB (73) | early | − | − | − | ||||||
|
|
|||||||||||
| 1211 | OBA (51) | (I) | − | − | −25.20 ± 2.11 | <17 | N | B? | N | N | N |
| 1211 | OBA-2 (42) | (I) | − | − | −6.88 ± 1.97 | <17 | |||||
| 1211 | OBB (51) | (I) | − | − | −12.25 ± 2.39 | <17 | |||||
| 1211 | OBB-2 (42) | (I) | − | − | −8.29 ± 7.35 | 33.9 ± 5.9 | |||||
| 1211 | OBC (49) | (I) | − | − | −10.66 ± 4.23 | <17 | |||||
| 1211 | OBC-2 (42) | (I) | − | − | −7.01 ± 6.72 | 34.4 ± 5.4 | |||||
|
|
|||||||||||
| 12 168 | OBA (52) | (I) | − | 185 | −33.92 ± 2.29 | 17.6 ± 1.2 | N | B? | Y | N | Y |
| 12 168 | OBA-2 (72) | (I) | − | −17.34 ± 2.11 | 21.5 ± 1.3 | ||||||
| 12 168 | OBC (62) | (I) | − | −21.30 ± 2.10 | <17 | ||||||
|
|
|||||||||||
| 1233 | OBA-2 (30) | (I) | − | − | −20.37 ± 2.30 | 19.9 ± 1.3 | N | N | N | N | N |
| 1233 | OBB-2 (40) | (I) | − | − | −20.80 ± 2.35 | 22.3 ± 1.5 | |||||
| 1233 | OBC-2 (40) | (I) | − | − | −21.04 ± 2.57 | 21.2 ± 1.5 | |||||
|
|
|||||||||||
| 12 631 | OBA (63) | (I) | − | − | −20.85 ± 2.02 | 17.9 ± 1.1 | N | B? | N | N | N |
| 12 631 | OBA-2 (76) | (I) | − | − | −4.09 ± 2.33 | 21.0 ± 1.4 | |||||
| 12 631 | OBB (63) | (I) | − | − | −9.33 ± 2.14 | <17 | |||||
| 12 631 | OBB-2 (73) | (I) | − | − | −4.85 ± 1.88 | <17 | |||||
| 12 631 | OBC (70) | (I) | − | − | −9.63 ± 3.33 | <17 | |||||
| 12 631 | OBC-2 (73) | (I) | − | − | −6.20 ± 2.12 | <17 | |||||
|
|
|||||||||||
| 1320 | OBA-2 (40) | early | − | −10.06 ± 5.87 | 20.4 ± 3.4 | N | Y | N | early | ? | |
| 1320 | OBB-2 (33) | early | − | −9.49 ± 5.85 | 17.6 ± 3.0 | ||||||
| 1320 | OBC-2 (33) | early | − | −9.57 ± 5.47 | 18.1 ± 2.9 | ||||||
|
|
|||||||||||
| 13 310 | OBA (69) | (I) | − | −18.24 ± 3.49 | 37.2 ± 2.9 | Y | N | Y | N | Y | |
| 13 310 | OBB (64) | (I) | − | −6.86 ± 1.75 | 33.3 ± 1.4 | ||||||
| 13 310 | OBC (60) | (I) | − | 284 | − | − | |||||
|
|
|||||||||||
| 1336 | OBA (41) | IV-B | 2.7−3.4 | − | −32.84 ± 2.28 | 17.7 ± 1.2 | N | B? | N | Y | ? |
| 1336 | OBA-2 (34) | IV-B | − | −15.75 ± 2.38 | 17.1 ± 1.2 | ||||||
| 1336 | OBB (42) | IV-B | − | −21.01 ± 2.56 | 20.0 ± 1.5 | ||||||
| 1336 | OBB-2 (38) | IV-B | − | −15.55 ± 2.37 | 19.6 ± 1.3 | ||||||
| 1336 | OBC (33) | (I asymm.) | − | −19.45 ± 3.56 | 17.8 ± 1.9 | ||||||
| 1336 | OBC-2 (38) | IV-B | − | −15.71 ± 2.29 | <17 | ||||||
|
|
|||||||||||
| 13 407 | OBB-2 (98) | (I) | 3.6 | − | −44.17 ± 2.53 | 20.3 ± 1.5 | N | N | N (V?) | Y | Y |
| 13 407 | OBC (65) | IV-B | − | −48.29 ± 2.39 | 22.3 ± 1.5 | ||||||
| 13 407 | OBC-2 (98) | (I) | − | −43.97 ± 2.80 | 22.2 ± 1.7 | ||||||
|
|
|||||||||||
| 1455 | OBA-2 (41) | IV-Bm | 4.1−4.4 | − | − | − | N | N | N (V?) | Y | Y |
| 1455 | OBB-2 (36) | IV-Bm | − | −52.09 ± 3.52 | 23.2 ± 2.3 | ||||||
| 1455 | OBC-2 (36) | IV-Bm | − | −51.31 ± 3.47 | 24.7 ± 2.3 | ||||||
|
|
|||||||||||
| 15 584 | OBA (86) | III-Bm | 11.6−14.6 | 324 (OBA, OBC) | −10.88 ± 2.06 | 40.0 ± 1.8 | Y | B? | Y | Y | Y |
| 15 584 | OBB (86) | IV-Bm + III-R | 0.32 ± 3.33 | 38.7 ± 2.8 | |||||||
| 15 584 | OBC (92) | IV-Bm | 0.94 ± 2.12 | 41.0 ± 1.8 | |||||||
|
|
|||||||||||
| 15 805 | OBA-2 (90) | (I) | − | 392 (OBA-2, OBC-2) | 5.64 ± 2.35 | 40.7 ± 2.0 | Y | Y | Y | N | Y |
| 15 805 | OBB-2 (94) | (I) | − | 8.17 ± 3.04 | 43.1 ± 2.7 | ||||||
| 15 805 | OBC-2 (94) | (I) | − | 5.55 ± 2.79 | 42.5 ± 2.4 | ||||||
|
|
|||||||||||
| 15 806 | OBA (96) | (I) | − | 448 | −18.65 ± 3.14 | 34.7 ± 2.5 | Y | B? | Y | N | Y |
| 15 806 | OBB (85) | (I) | − | −7.18 ± 2.7 | 31.1 ± 2.1 | ||||||
| 15 806 | OBC (86) | (I) | − | −7.39 ± 2.16 | 33.7 ± 1.7 | ||||||
|
|
|||||||||||
| 2062 | OBA (40) | III-B or Rm | 17.9−21.3 | − | − | − | N | − | N (V) | Y | Y |
| 2062 | OBA-2 (29) | III-B or Rm | − | − | − | ||||||
| 2062 | OBB (40) | III-B or Rm | − | − | − | ||||||
| 2062 | OBB-2 (24) | III-B or Rm | − | − | − | ||||||
| 2062 | OBC (37) | III-B or Rm | − | − | − | ||||||
| 2062 | OBC-2 (24) | III-B or Rm | − | − | − | ||||||
|
|
|||||||||||
| 2594 | OBA-2 (3) | IV-Bm | 4.3−11.4 | − | −48.75 ± 3.13 | <17 | N | N | N | Y | ? |
| 2594 | OBB-2 (4) | III-Bm | − | −47.82 ± 5.61 | 25.3 ± 3.8 | ||||||
| 2594 | OBC-2 (4) | II-Bm | − | −47.59 ± 5.77 | 23.8 ± 3.8 | ||||||
|
|
|||||||||||
| 4112 | OBA (7) | IV-Rm | 3.3−4.7 | − | 36.98 ± 2.68 | 26.9 ± 1.9 | N | SB2 | N | Y | ? |
| 4112 | OBB (7) | IV-Rm | − | 50.23 ± 2.90 | 23.1 ± 1.8 | ||||||
| 4112 | OBC (5) | IV-Rm | − | 50.62 ± 3.50 | 20.6 ± 2.1 | ||||||
Notes. ID of each BWE star; OB in which each BWE star has been observed (number of the spectrum in brackets); Hα profile type (in brackets the profiles not visible because of the nebular influence, as explained in the text); FWZI of this emission line (− if the profile is within the nebular range); EW(Li); RV and vsin(i) (− for cases in which there are not enough lines that can be used in FXCOR). In bold are highlighted the objects showing a variable RV. Detection in X-rays (− if outside of the field of view); total membership using the criteria: Li > 100 mÅ, and Hα emission line (N (V?): veiling?; Y: YES; N: NO; SKY: emission line within the λ range effected by the nebular emission, B?: binary?; SB2: binary system with the two components resolved); the values that are the same for each of the OBs are shown in the first OB in which the star is detected; otherwise is indicated.
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