Table B.2
Photometric properties of all the W-R stars in 30 Dor.
| ID | Star | Spectral | Ref. | m v | b − v | Ref. | Wλ(4686) | Wλ(5808) | Ref. | (b − v)0 | R v a | A v |
|
ΔMv |
|
||||
| # | BAT99 | VFTS | Alias | Type | [mag] | [mag] | [Å] | [Å] | [mag] | [mag] | [mag] | [mag] | [mag] | ||||||
|
|
|||||||||||||||||||
| 24 | 86 | 019 | Br 69 | WN 3(h) | (1)b | 16.68 | 0.11 | (11) | 110 | – | (1) | −0.27 | 4.6 | 1.7 | −3.6 | – | – | ||
| 92 | 88 | 079 | Br 70a | WN 4b/WCE | (2) | 17.75 | 0.46 | (12) | 225 | 1660 | (1,12) | −0.23 | 4.6 | 3.2 | −3.9 | – | – | ||
| 117 | 89 | 108 | Br 71 | WN 7h | (3) | 14.13 | 0.22 | (3) | 96 | – | (1) | −0.28 | 4.6 | 2.3 | −6.7 | – | – | ||
| 144 | 90 | 136 | Br 74 | WC 4 | (4) | 15.42 | 0.12 | (12) | – | 1451 | (12) | −0.16 | 4.6 | 1.3 | −4.4 | – | – | ||
| 155 | 91 | 147 | Br 73-1A | WN 6(h) | (1) | 14.98 | 0.15 | (13) | 39 | – | (1) | −0.30 | 4.6 | 2.1 | −5.6 | – | – | ||
| 185 | 92 | Br 72, R130 | WCE/WN+B1 I | (5) | 11.47 | 0.03 | (11) | 14 | 73 | (14,18) | −0.31 | 4.6 | 1.6 | −8.6 | + 3.2c | −5.4 | |||
| 375 | 95 | 402 | Br 80, R135 | WN 7h+OB | (1) | 13.04 | 0.09 | (3,14) | 80 | – | (1) | −0.28 | 4.6 | 1.7 | −7.2 | −3.5 | −7.2 | ||
| 402 | 96 | 427 | Br 81 | WN 8(h) | (3) | 13.82 | 0.49 | (3) | 40 | – | (1) | −0.30 | 4.6 | 3.6 | −8.3 | – | – | ||
| 443 | 98 | Br 79, Mk 49 | WN 6(h) | (6) | 13.37 | 0.10 | (3) | 19 | – | (18) | −0.31 | 4.6 | 1.9 | −7.0 | – | – | |||
| 493 | 100 | 1001 | Br75, R134 | WN 7h | (3) | 12.40 | 0.14 | (3) | 27 | – | (18) | −0.31 | 5.4 | 2.4 | −8.5 | – | – | ||
| 543 | 101 | 507 | Br 87, R140a1 | WC 4(+WN 6+O) | (7) | { | 12.50 | 0.03 | (16,17) | – | 170d | (1) | –0.32 | 4.6 | 1.6 | −7.6 | +2.0 | −5.5 | |
| 544 | 102 | 507 | Br 87, R140a2 | WN 6+(O) | (8) | 12.50 | 0.03 | (16,17) | 53 | – | (1) | −0.31 | 4.6 | 1.6 | −7.6 | −1.0 | −7.2 | ||
| 545 | 103 | 509 | Br 87, R140b | WN 5(h)+O(+early O) | (1) | 12.80 | 0.03 | (16,17) | 42 | – | (1) | −0.30 | 4.6 | 1.5 | −7.2 | −0.3 | −6.6 | ||
| 613 | 106 | Br 82, R136a3 | WN 5h | (6) | 13.02 | 0.05 | (15) | 55 | – | (15) | −0.29 | 5.4 | 1.8 | −7.3 | – | – | |||
| 630 | 108 | Br 82, R136a1 | WN 5h | (6) | 12.23 | 0.03 | (15) | 37 | – | (15) | −0.30 | 5.4 | 1.8 | −8.1 | – | – | |||
| 633 | 109 | Br 82, R136a2 | WN 5h | (6) | 12.77 | 0.06 | (15) | 41 | – | (15) | −0.30 | 5.4 | 2.0 | −7.7 | – | – | |||
| 706 | 112 | 1025 | Br 82, R136c | WN 5h | (6) | 13.39 | 0.20 | (9,17) | 54 | – | (15) | −0.30 | 5.4 | 2.7 | −7.8 | – | – | ||
| 762 | 115 | Br 83, Mk33Sb | WC 5 | (9) | 15.23 | 0.12 | (9) | – | 1100d | (9) | –0.28 | 5.4 | 2.2 | −5.4 | – | – | |||
| 770 | 116 | Br 84, Mk34 | WN 5h | (6) | 13.10 | 0.14 | (9,17) | 30 | – | (18) | −0.33 | 5.4 | 2.6 | −7.9 | – | – | |||
| 862 | 117 | 617 | Br 88, R146 | WN 5ha | (2) | 12.95 | −0.16 | (12) | 37 | – | (1) | −0.30 | 4.6 | 0.6 | −6.2 | – | – | ||
| 916 | 118 | Br 89 | WN 6he | (10) | 11.20 | −0.17 | (11) | 60 | – | (18) | −0.29 | 4.6 | 0.6 | −7.8 | – | – | |||
| 928 | 118a | 682 | WN 5h | (1) | 16.30 | 0.60 | (1,16) | 39 | – | (1) | −0.30 | 4.6 | 4.1 | −6.3f | – | – | |||
| 938 | 119 | 695 | Br 90, R145 | WN 6h+? | (1) | 12.06 | 0.03 | (11) | 39 | – | (1) | −0.30 | 4.6 | 1.5 | −7.9 | −0.1 | −7.2 | ||
| 973 | 121 | 731 | Br 90a | WC 4 | (4) | 17.21 | 0.31 | (12) | – | 1258 | (12) | −0.28 | 4.6 | 2.8 | −4.1 | – | – | ||
| 1001 | 122 | 758 | Br 92, R147 | WN 5h | (1) | 12.75 | 0.03 | (12) | 76 | – | (1) | −0.29 | 4.6 | 1.5 | −7.2 | – | – | ||
Notes. Values in italic indicate where magnitudes
or colours have been assumed. The
Wλ of the He ii
λ4686 line for WN stars or C iv
λ5808 line for WC stars, is listed with references. For
multiple systems, a magnitude correction is given, where 
. Note that the template W-R stars will have had different
Av and
values derived from their CMFGEN
models, as listed in Table B.1, and that
the properties given in that table are adopted for the star. Similarly, for
comparison, this table gives photometry for stars BAT99-90, 106, 108, 109, 112
but their stellar properties were equivalently adopted from Crowther et al. (2002) or Crowther et al. (2010) and were not derived
from the values in this table. See text for more details. The photometric data
given for stars BAT99-101 and 102 are for the combined R140a system.
Narrow band Rv derived from average broadband RV determined for each region (see Appendix C).
Revealed as a WN 5-6+WN 6-7 binary system by Sana et al. (2013b).
was estimated using broad band
photometry and v − V ≈ 0.2 mag relation from Breysacher (1986). However, high reddening
allows for a large uncertainty and the star is thought to be more comparable
to BAT99-106 (F. Najarro).
Reference. (1) Paper I; (2) Foellmi et al. (2003); (3) Crowther & Smith (1997); (4) Smith et al. (1990); (5) Conti & Massey (1989); (6) Crowther & Dessart (1998); (7) Bartzakos et al. (2001); (8) Moffat et al. (1987); (9) Massey & Hunter (1998); (10) Smith et al. (1996); (11) Schmutz & Vacca (1991); (12) Crowther & Hadfield (2006); (13) Walborn et al. (1999); (14) Torres-Dodgen & Massey (1988); (15) de Koter et al. (1997), (16) Breysacher (1986); (17) De Marchi et al. (2011); (18) Schnurr et al. (2008).
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