Table A.1
Best fit parameters and 1er error barsa) for the optical + UV fits of 39 stars where we fitted 12 free parameters.
| Source | log L/L⊙ | Teff(K) | log g | R*/R⊙ | log  |
υ∞ (km/s) | υwindturb/υ∞ | fcl | fic | fvel | β | υcl,start/υ∞ |  |
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|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| R136a1b) |  |
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| R136a2b) |  |
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| R136a3b,c) |  |
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| R136a4 |  |
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| R136a5 |  |
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| R136a6 |  |
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| R136a7 |  |
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| R136a8 |  |
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| R136b |  |
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| H30 |  |
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| H31 |  |
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| H35 |  |
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| H36 |  |
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| H40 |  |
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| H45 |  |
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| H46 |  |
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| H47 |  |
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| H48 |  |
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| H49 |  |
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| H50 |  |
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| H52 |  |
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| H55 |  |
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| H58 |  |
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| H62 |  |
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| H64 |  |
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| H65 |  |
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| H66 |  |
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| H68 |  |
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| H69 |  |
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| H70 |  |
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| H71 |  |
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| H75 |  |
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| H78 |  |
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| H80 |  |
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| H86 |  |
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| H90 |  |
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| H92 |  |
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| H94 |  |
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| H143 |  |
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a) It is important to note that when the error bar reaches the edge of the parameter space, the best fit value is in fact an upper or lower limit. Figure 8 shows when this is the case.
b) Run with 14 free parameters. Values for the helium and oxygen surface abundance can be found in Table A.3.
c) Formal uncertainties from the KIWI-GA run with fixed, estimated Teff of 50 kK (see text). In reality uncertainties on all parameters for this source are larger due to the uncertain Teff.
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