Table 3
Stellar properties derived from best-fit FASTWIND parameters and the SED fitting.
Name | Sp. Type | Sp. Type | Teff | log g | vsini | RV | AV | log L/L⊙ | R⋆ | Mspec | RV |
Hanson | This work | K | cm s-2 | km s-1 | (SED) | mag | R⊙ | M⊙ | km s-1 | ||
|
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B111 | O5 V | O4.5 V |
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3.4 ± 0.8 |
B163 | ? | kA5 | 8200 | − | − |
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− | − |
B164 | O7-O8 | O6 Vz |
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–1.8 ± 2.3 |
B215 | B0.5 V | B0-B1 V |
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12.3 ± 1.0 |
B243 | B3 V | B8 V |
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20.2 ± 1.5 |
B253 | B3V | B3-B5 III |
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9.5 ± 0.8 |
B268 | B2 V | B9-A0 |
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4.3 ± 1.3 |
B275 | late-Ob | B7 III |
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–11.2 ± 1.4 |
B289 | O9.5 V | O9.7V |
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-2.3 ± 2.0 |
B311 | O9-B2 V | O8.5 Vz |
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4.2 ± 0.4 |
B331 | B2 Vc | late-B | 13 000 | − | − |
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− | 13.9 ± 1.5 |
B337 | mid-Bb | late-B | 13 000 | − | − |
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− | 7.5 ± 0.6 |
Notes. The values for the stellar radius (R⋆) cited here are those obtained via SED fitting. The sources classified as PMS stars in this work are in bold face and the two sources for which we cannot confirm the PMS nature are underlined.
From SED in H97.
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