Table A.1
Comparison of basic stellar parameters of Wd1-5 to those of related galactic stars.
| Name | Spec. | log(L∗) | R∗ | Teff | log g | log(Ṁ) | v∞ | Reference |
| Type | (L⊙) | (R⊙) | (kK) | (M⊙ yr-1) | (kms-1) | |||
|
|
||||||||
| Wd1-5 | B0.5 Ia+ |
|
|
|
|
|
|
This work |
| HD 30614 | O9.5 Ia | 5.63 | 26.0 | 29.0 ± 1.0 | 3.0 ± 0.15 |
|
1560 | 1 |
| HD 168183 | O9.5 Ib | 5.42 ± 0.22 |
|
30.0 ± 1.0 | 3.3 ± 0.1 |
|
1700 ± 510 | 2 |
| HD 37128 | B0 Ia | 5.44 | 24.0 | 27.0 ± 1.0 | 2.9 ± 0.15 |
|
1910 | 1 |
| HD 89767 | B0 Ia | 5.35 ± 0.22 |
|
23.0 ± 1.0 | 2.55 ± 0.1 |
|
1600 ± 480 | 2 |
| HD 91969 | B0 Ia | 5.52 | 25.3 | 27.5 ± 1.0 | 2.75 ± 0.14 |
|
1470 | 1 |
| HD 94909 | B0 Ia | 5.49 | 25.5 | 27.0 ± 1.0 | 2.9 ± 0.14 |
|
1050 | 1 |
| HD 122879 | B0 Ia | 5.52 | 24.4 | 28.0 ± 1.0 | 2.95 ± 0.14 |
|
1620 | 1 |
| HD 192660 | B0 Ib | 5.74 ± 0.13 | 23.4 ± 1.0 | 30.0 ± 1.0 | 3.25 |
|
1850 | 3 |
| HD 204172 | B0.2 Ia | 5.48 ± 0.27 | 22.4 ± 3.2 | 28.5 ± 1.0 | 3.13 |
|
1685 | 3 |
| HD 38771 | B0.5 Ia | 5.35 | 22.2 | 26.5 ± 1.0 | 2.9 ± 0.14 |
|
1525 | 1 |
| HD 115842 | B0.5 Ia | 5.65 | 34.2 | 25.5 ± 1.0 | 2.85 ± 0.14 |
|
1180 | 1 |
| HD 152234 | B0.5 Ia | 5.87 | 42.4 | 26.0 ± 1.0 | 2.85 ± 0.14 |
|
1450 | 1 |
| HD 185859 | B0.5 Ia | 5.54 ± 0.14 | 29.1 ± 1.3 | 26.0 ± 1.0 | 3.13 |
|
1830 | 3 |
| HD 64760 | B0.5 Ib | 5.48 ± 0.26 | 23.3 ± 2.2 | 28.0 ± 2.0 | 3.38 |
|
1600 | 3 |
| HD 93619 | B0.5 Ib | 5.30 ± 0.22 |
|
26.0 ± 1.0 | 2.9 ± 0.1 |
|
1470 ± 441 | 2 |
| HD 213087 | B0.5 Ib | 5.69 ± 0.11 | 32.0 ± 0.01 | 27.0 ± 1.0 | 3.13 |
|
1520 | 3 |
| HD 2905 | BC0.7 Ia | 5.52 | 41.4 | 21.5 ± 1.0 | 2.6 ± 0.14 |
|
1105 | 1 |
| HD 91943 | B0.7 Ia | 5.35 | 26.3 | 24.5 ± 1.0 | 2.8 ± 0.14 |
|
1470 | 1 |
| HD 152235 | B0.7 Ia | 5.76 | 47.1 | 23.0 ± 1.0 | 2.65 ± 0.14 |
|
850 | 1 |
| HD 154090 | B0.7 Ia | 5.48 | 36.0 | 22.5 ± 1.0 | 2.65 ± 0.14 |
|
915 | 1 |
| HD 96880 | B1 Ia | 5.42 ± 0.11 |
|
20.0 ± 1.0 | 2.4 ± 0.1 |
|
1200 ± 360 | 2 |
| HD 115363 | B1 Ia | 5.42 ± 0.11 |
|
20.0 ± 1.0 | 2.4 ± 0.1 |
|
1200 ± 360 | 2 |
| HD 148688 | B1 Ia | 5.45 | 36.7 | 22.0 ± 1.0 | 2.60 ± 0.14 |
|
725 | 1 |
| HD 170938 | B1 Ia | 5.42 ± 0.11 |
|
20.0 ± 1.0 | 2.4 ± 0.1 |
|
1200 ± 360 | 2 |
| HD 13854 | B1 Iab | 5.43 | 37.4 | 21.5 ± 1.0 | 2.55 ± 0.14 |
|
920 | 1 |
| HD 91316 | B1 Iab | 5.47 | 37.4 | 22.0 ± 1.0 | 2.55 ± 0.14 |
|
1110 | 1 |
| HD 109867 | B1 Iab | 5.56 ± 0.22 |
|
23.0 ± 1.0 | 2.6 ± 0.1 |
|
1400 ± 420 | 2 |
| HD 190066 | B1 Iab | 5.54 ± 0.20 | 41.4 ± 1.9 | 21.0 ± 1.0 | 2.88 |
|
1275 | 3 |
| HD 47240 | B1 Ib | 4.93 ± 0.22 |
|
19.0 ± 1.0 | 2.4 ± 0.1 |
|
1000 ± 300 | 2 |
| HD 154043 | B1 Ib | 4.98 ± 0.22 |
|
20.0 ± 1.0 | 2.5 ± 0.1 |
|
1300 ± 390 | 2 |
| HD 54764 | B1 Ib/II | 4.90 ± 0.22 |
|
19.0 ± 1.0 | 2.45 ± 0.10 |
|
900 ± 270 | 2 |
| HD 14956 | B1.5 Ia | 5.65 | 50.6 | 21.0 ± 1.0 | 2.5 ± 0.14 |
|
500 | 1 |
| HD 106343 | B1.5 Ia | 5.40 ± 0.22 |
|
20.0 ± 1.0 | 2.50 ± 0.1 |
|
800 ± 240 | 2 |
| HD 193183 | B1.5 Ib | 5.00 ± 0.26 | 30.8 ± 2.8 | 18.5 ± 1.0 | 2.63 |
|
565 | 3 |
| HD 111990 | B1/2 Ib | 4.91 ± 0.22 |
|
19.5 ± 1.0 | 2.55 ± 0.10 |
|
750 ± 225 | 2 |
| HD 14143 | B2 Ia | 5.42 | 52.9 | 18.0 ± 1.0 | 2.25 ± 0.14 |
|
645 | 1 |
| HD 14818 | B2 Ia | 5.35 | 46.1 | 18.5 ± 1.0 | 2.4 ± 0.14 |
|
565 | 1 |
| HD 41117 | B2 Ia | 5.65 | 61.9 | 19.0 ± 1.0 | 2.35 ± 0.14 |
|
510 | 1 |
| HD 194279 | B2 Ia | 5.37 | 44.7 | 19.0 ± 1.0 | 2.3 ± 0.14 |
|
550 | 1 |
| HD 206165 | B2 Ib | 5.18 ± 0.26 | 39.8 ± 5.5 | 18.0 ± 0.5 | 2.50 |
|
640 | 3 |
| HD 141318 | B2 II | 4.56 ± 0.11 | 16.0 | 20.0 ± 1.0 | 2.90 ± 0.1 |
|
900 ± 270 | 2 |
| HD 92964 | B2.5 Iae | 5.33 ± 0.11 | 48.0 | 18.0 ± 1.0 | 2.1 ± 0.1 |
|
520 ± 156 | 2 |
| HD 198478 | B2.5 Ia | 5.03 | 40.0 | 16.5 ± 1.0 | 2.15 ± 0.14 |
|
470 | 1 |
| HD 42087 | B2.5 Ib | 5.11 ± 0.24 | 36.6 ± 1.7 | 18.0 ± 1.0 | 2.50 |
|
650 | 3 |
| HD 14134 | B3 Ia | 5.28 | 56.7 | 16.0 ± 1.0 | 2.05 ± 0.14 |
|
465 | 1 |
| HD 53138 | B3 Ia | 5.34 | 65.0 | 15.5 ± 1.0 | 2.05 ± 0.14 |
|
865 | 1 |
| HD 58350 | B5 Ia | 5.18 ± 0.17 | 57.3 ± 2.6 | 15.0 ± 0.5 | 2.13 |
|
320 | 3 |
| HD 102997 | B5 Ia | 5.25 ± 0.22 |
|
16.0 ± 1.0 | 2.00 ± 0.1 |
|
325 ± 98 | 2 |
| HD 108659 | B5 Ib | 4.60 ± 0.22 |
|
16.0 ± 1.0 | 2.30 ± 0.1 |
|
470 ± 141 | 2 |
| HD 164353 | B5 Ib | 4.30 ± 1.30 | 19.6 ± 8.1 | 15.5 ± 1.0 | 2.75 |
|
450 | 3 |
| HD 80558 | B6 Iab | 4.78 ± 0.22 |
|
13.5 ± 1.0 | 1.75 ± 0.1 |
|
250 ± 75 | 2 |
| HD 91024 | B7 Iab | 4.74 ± 0.22 |
|
12.5 ± 1.0 | 1.95 ± 0.1 |
|
225 ± 68 | 2 |
| HD 199478 | B8 Iae | 5.08 | 68.0 | 13.0 ± 1.0 | 1.70 | -6.70...-6.15 | 230 | 4 |
| HD 94367 | B9 Ia | 4.97 ± 0.22 |
|
11.5 ± 1.0 | 1.55 ± 0.1 |
|
175 ± 53 | 2 |
| HD 202850 | B9Iab | 4.59 ± 0.22 | 54.0 | 11.0 ± 1.0 | 1.85 |
|
240 | 4 |
| HD 212593 | B9 Iab | 4.79 ± 0.22 | 59.0 | 11.8 ± 1.0 | 2.18 |
|
350 | 4 |
| BP Cru | B1 Ia+ | 5.67 | 70.0 |
|
2.38 | -5.00 | 305 | 5 |
| ζ1 Sco | B1.5 Ia+ | 5.93 | 103.0 | 17.2 ± 0.5 | 1.97 | -5.2 | 390 ± 50 | 6 |
| HD 190603 | B1.5 Ia+ | 5.58 | 63.0 | 18.0 ± 0.5 | 2.10 | -5.66 | 485 ± 50 | 6 |
| Cyg #12 | B3-4 Ia+ | 6.28 | 246.0 |
|
|
-4.82 |
|
6 |
| AG Car | LBV |
|
58.5 | 22.8 ± 0.5 | - |
|
300 ± 30 | 7 |
|
115.2 | 14.3 ± 0.5 | - |
|
150 ± 30 | 7 | ||
| P Cygni | LBV | 5.85 | 76.0 | 19.2 | - | -4.49 | 185 | 8 |
| HR Car | LBV | 5.70 | 70.0 | 17.9 | - | -4.85 | 120 | 9 |
| Pistol star | LBV | 6.20 | 306 | 11.8 ± 1.5 | - | -4.12 | 105 | 10 |
| FMM 362 | LBV | 6.25 | 350 | 11.3 ± 1.5 | - | -4.37 | 170 | 10 |
| AFGL2298 | LBV | 6.30 | 385 | 11.0 ± 0.5 | - | -4.28 | 125 | 11 |
| NS4 | WNLh | 5.58 | 22.6 | 28.4 | - | -4.35 | 700 | 12 |
| HD 313846 | WNLh | 5.82 | 33.1 | 27.7 | - | -4.53 | 1170 | 12 |
| GC AF | WNLh | 5.3 ± 0.2 | 28.1 ± 0.6 | 21.0 | - | −4.25 ± 0.2 | 700 ± 100 | 13 |
| GC IRS16C | WNLh | 5.9 ± 0.2 | 63.9 | 19.5 ± 6.0 | - | −4.65 ± 0.2 | 650 ± 100 | 13 |
| GC IRS34W | WNLh | 5.5 ± 0.2 | 35.9 | 19.5 ± 6.0 | - | −4.88 ± 0.2 | 650 ± 100 | 13 |
| GC IRS33E | WNLh | 5.75 ± 0.2 | 63.9 | 18.0 ± 6.0 | - | −4.80 ± 0.2 | 450 ± 100 | 13 |
| GC IRS19NW | WNLh | 5.9 ± 0.2 | 59.1 | 17.5 ± 6.0 | - | −4.95 ± 0.2 | 600 ± 100 | 13 |
Notes. Stars are presented from early to late spectral types for BSGs and BHGs and from hottest to coolest for the LBVs and WNLh stars. The lack of suitable absorption profiles prevents a determination of the surface gravity of the LBVs and WNLh stars. Throughout the table we employ the clumping corrected mass loss rate (Ṁ/
) to allow direct comparison between individual stars; hence the difference between this table and Table 1 for Wd1-5. Unfortunately errors are not presented for all physical parameters of all individual stars by the studies used in the construction of this table. Values for both high and low temperature states of AG Car are provided.
Reference.
Crowther et al. (2006b);
Lefever et al. (2007);
Searle et al. (2008);
Markova & Puls (2008);
Kaper et al. (2006);
Clark et al. (2012);
Groh et al. (2009a);
Najarro (2001);
Groh et al. (2009b);
Najarro et al. (2009);
Clark et al. (2009b);
Bohannan & Crowther (1999);
Martins et al. (2007).
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