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Table 3
Results from the time-dependent line-broadening analysis of a sample of eight O and B stars with an important contribution of non-rotational sources of line broadening.
| # | Star | Sp. C | N | ν sin i | νmac | log Teff | log L/ L⊙ | Notes | |||||
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|
σ x | Range |
|
σ x | Range | ||||||||
| O stars and B Sgs (OB stars) with multi-epoch observations gathered in the framework of the IACOB project | |||||||||||||
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|
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| 1 | HD 199579 | O6.5 V((f))z | 112 | 56.2 | 8% | [48.0, 69.0] | 81.2 | 7% | [65.0, 90.4] | 4.60 | 3.83 | SB1 | |
| 2 | HD 36861 | O8 III | 172 | 54.2 | 3% | [49.4, 60.0] | 73.2 | 4% | [64.3, 80.0] | 4.55 | 4.06 | – | |
| 3 | HD 38771 | B0 Iab | 154 | 61.5 | 7% | [49.6, 71.4] | 82.5 | 6% | [67.5, 95.2] | 4.47 | 4.06 | – | |
| 4 | HD 34085 | B8 Iab | 108 | 38.7 | 7% | [32.3, 47.6] | 52.9 | 10% | [47.1, 67.5] | 4.10 | 4.10 | – | |
| B main-sequence stars from the study by Aerts et al. (2014) | |||||||||||||
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| 5 | HD 111123 | B0.5 IV | 119 | 28.6 | 22% | [16.5, 41.9] | 42.8 | 11% | [33.1, 57.3] | 4.43 | 3.42 | SB1, nr-p | |
| 6 | HD 16582 | B2 IV | 59 | 11.6 | 23% | [4.1, 16.1] | 17.7 | 10% | [12.7, 20.8] | 4.36 | 3.04 | r | |
| 7 | HD 105382 | B6 III | 106 | 68.3 | 10% | [49.6, 78.8] | 27.6 | 40% | [10.8, 73.0] | 4.24 | 2.15 | spot | |
| 8 | HD 181558 | B5 III | 30 | 4.1 | 100% | [0, 24.7] | 15.4 | 48% | [ 0.0, 27.8] | 4.17 | 1.86 | nr-g | |
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