Table B.1
Best-fit values of the R136 core stars†.
| Source | RV | AV | AK | log L/L⊙ | c2 | c4 |  |
|---|---|---|---|---|---|---|---|
| R136a1 | 4.25±0.10 | 1.85±0.02 | 0.24 | 6.82 ± 0.01 | 1.28±0.05 |  |
4.44 |
| R136a2 | 2.93±0.15 | 1.25±0.04 | 0.14 | 6.59 ± 0.01 | 1.62±0.11 |  |
14.32 |
| R136a3 | 4.63±0.08 | 1.99±0.02 | 0.26 | 6.69 ± 0.01 | 1.14±0.03 |  |
1.81 |
| R136a4 | 3.30±0.14 | 1.38±0.03 | 0.17 | 6.23 ± 0.01 | 1.43±0.07 |  |
4.83 |
| R136a5 | 4.67±0.31 | 2.00±0.05 | 0.27 | 6.34 ± 0.01 | 1.33±0.13 |  |
13.18 |
| R136a7 | 5.04±0.61 | 1.82±0.07 | 0.25 | 6.29 ± 0.02 | 1.87±0.30 |  |
24.60 |
| R136b | 5.66±0.21 | 2.57±0.04 | 0.36 | 6.39 ± 0.01 | 1.18±0.08 |  |
8.72 |
| H30 | 4.13±0.13 | 1.63±0.03 | 0.21 | 5.72 ± 0.01 | 1.15±0.06 |  |
3.90 |
| H31 | 3.94±0.24 | 1.53±0.05 | 0.20 | 5.93 ± 0.02 | 1.24±0.13 |  |
19.94 |
| H35 | 4.66±0.29 | 1.57±0.04 | 0.21 | 5.81 ± 0.01 | 1.34±0.09 |  |
5.69 |
| H36 | 5.79±0.31 | 2.63±0.05 | 0.37 | 6.31 ± 0.02 | 1.15±0.12 |  |
17.16 |
| H40 | 5.55±0.41 | 1.95±0.06 | 0.27 | 5.93 ± 0.02 | 1.30±0.15 |  |
20.02 |
| H45 | 5.38±0.13 | 2.20±0.02 | 0.30 | 5.82 ± 0.01 | 1.25±0.06 |  |
3.39 |
| H46 | 5.04±0.32 | 2.38±0.06 | 0.32 | 6.12 ± 0.02 | 1.18±0.19 |  |
23.42 |
| H47 | 5.47±0.52 | 2.50±0.09 | 0.35 | 5.99 ± 0.03 | 1.15±0.31 |  |
39.86 |
| H48 | 5.42±0.37 | 2.31±0.06 | 0.32 | 5.98 ± 0.01 | 1.21±0.13 |  |
13.09 |
| H50 | 4.17±0.10 | 1.83±0.02 | 0.24 | 5.84 ± 0.00 | 1.11±0.04 |  |
1.59 |
| H52 | 4.80±0.23 | 1.67±0.03 | 0.23 | 5.69 ± 0.01 | 1.29±0.10 |  |
4.87 |
| H55 | 4.66±0.38 | 1.73±0.06 | 0.23 | 5.76 ± 0.02 | 1.27±0.16 |  |
18.26 |
| H58 | 4.96±0.41 | 2.06±0.06 | 0.28 | 5.87 ± 0.01 | 1.31±0.18 |  |
13.36 |
| H62 | 4.54±0.17 | 1.68±0.02 | 0.22 | 5.61 ± 0.01 | 1.18±0.06 | 0 21 ± 0 14 | 1.86 |
| H64 | 5.23±0.45 | 2.35±0.08 | 0.32 | 5.85 ± 0.02 | 1.29±0.21 |  |
35.26 |
| H66 | 4.06±0.17 | 1.78±0.03 | 0.23 | 5.65 ± 0.01 | 1.12±0.07 | 0.25±0.19 | 2.27 |
| H68 | 5.21±0.13 | 2.34±0.02 | 0.32 | 5.69 ± 0.01 | 1.20±0.07 |  |
4.19 |
| H69 | 4.92±0.59 | 1.75±0.07 | 0.24 | 5.45 ± 0.01 | 1.46±0.14 |  |
1.19 |
| H70 | 4.18±0.45 | 1.85±0.08 | 0.24 | 5.68 ± 0.02 | 1.34±0.28 |  |
17.69 |
| H71 | 4.45±0.82 | 1.55±0.11 | 0.20 | 5.44 ± 0.03 | 1.35±0.33 |  |
43.68 |
| H73 | 3.68±0.23 | 1.65±0.04 | 0.21 | 5.15 ± 0.01 | 0.96±0.07 | 0.16±0.16 | 3.09 |
| H75 | 3.72±0.12 | 1.41±0.02 | 0.18 | 5.45 ± 0.00 | 1.40±0.06 | 0 17±0 14 | 1.34 |
| H78 | 4.59±0.24 | 1.71±0.03 | 0.23 | 5.50 ± 0.01 | 1.45±0.09 |  |
2.17 |
| H80 | 3.91±0.21 | 1.40±0.03 | 0.18 | 5.09 ± 0.01 | 1.19±0.08 |  |
2.30 |
| H86 | 2.36±0.60 | 1.06±0.14 | 0.11 | 5.42 ± 0.03 | 1.22±0.35 |  |
56.89 |
| H90 | 4.85±0.15 | 1.79±0.02 | 0.24 | 5.34 ± 0.00 | 1.31±0.05 |  |
0.52 |
| H92 | 4.66±0.16 | 1.64±0.02 | 0.22 | 5.21 ± 0.00 | 1.27±0.05 |  |
0.63 |
| H94 | 5.15±0.26 | 1.87±0.03 | 0.26 | 5.39 ± 0.01 | 1.39±0.08 |  |
1.44 |
| H108 | 1.91±0.26 | 0.77±0.06 | 0.07 | 4.88 ± 0.01 | 1.21±0.15 |  |
9.05 |
| H112 | 4.19±0.98 | 1.85±0.15 | 0.24 | 5.08 ± 0.03 | 1.16±0.35 |  |
24.59 |
| H114 | 4.64±0.69 | 1.55±0.08 | 0.21 | 5.21 ± 0.02 | 1.40±0.24 |  |
11.09 |
| H116 | 4.85±1.57 | 1.45±0.15 | 0.20 | 4.86 ± 0.03 | 1.54±0.54 |  |
37.99 |
| H120 | 2.36±0.88 | 0.93±0.20 | 0.09 | 4.78 ± 0.06 | 1.24±0.57 |  |
164.30 |
| H121 | 4.33±1.39 | 1.46±0.17 | 0.19 | 4.77 ± 0.03 | 1.24±0.48 |  |
48.33 |
| H123 | 3.39±0.87 | 1.22±0.14 | 0.15 | 4.87 ± 0.03 | 1.37±0.44 |  |
59.44 |
| H132 | 3.79±0.51 | 1.49±0.08 | 0.19 | 5.01 ± 0.01 | 1.22±0.19 |  |
7.05 |
| H134 | 4.16±1.38 | 1.27±0.16 | 0.16 | 4.72 ± 0.04 | 1.46±0.62 |  |
62.54 |
| H135 | 2.98±0.69 | 1.36±0.13 | 0.16 | 4.65 ± 0.02 | 0.78±0.20 |  |
10.99 |
| H139 | 4.67±1.13 | 1.47±0.13 | 0.20 | 4.90 ± 0.02 | 1.43±0.38 |  |
21.19 |
| H141 | 5.03±0.53 | 1.43±0.05 | 0.19 | 4.67 ± 0.01 | 2.36±0.30 |  |
2.21 |
| H143 | 3.75±0.62 | 1.75±0.11 | 0.22 | 5.11 ± 0.02 | 1.06±0.21 |  |
10.19 |
| H159 | 5.36±0.92 | 1.72±0.09 | 0.24 | 4.69 ± 0.01 | 1.47±0.32 |  |
7.74 |
| H173 | 3.54±0.54 | 1.18±0.07 | 0.15 | 4.42 ± 0.01 | 1.31±0.22 |  |
4.91 |
| Average | 4.38±0.87 | 1.71±0.41 | 0.22 | 1.30±0.22 | 0.09±0.08 | ||
† The parameters c2 and c4 correspond to the slope of the UV extinction, and the far-UV curvature, respectively. For all stars, we adopted c1 = 2.030 – 3.007c2; c3 = 1.463; c5 = 5.9, x0 = 4.558, and γ = 0.945. The uncertainties quoted here are statistical uncertainties resulting from the extinction fits; in the case of luminosity, the uncertainties associated with the derivation of stellar parameters (see Brands et al. (2022), their Table A.1.) are not included.
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