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Table A.2
Best fit parameters and 1σ error barsa) for the optical + UV fits of the 17 stars where we fitted six free parameters.
| Source | log L/L⊙ | Teff (K) | log g | R*/R⊙ | log  |
υ∞ (km/s) | fcl | β |
|---|---|---|---|---|---|---|---|---|
| H73 |  |
 |
 |
 |
 |
 |
 |
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| H108 |  |
 |
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| H112 |  |
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 |
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| H114 |  |
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| H116 |  |
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| H120 |  |
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| H121 |  |
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| H123 |  |
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| H129 |  |
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| H132 |  |
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| H134 |  |
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| H135 |  |
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| H139 |  |
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| H141 |  |
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| H159 |  |
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| H162 |  |
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| H173 |  |
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 |
a) We 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 9 shows when this is the case.
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