Table 2
Stellar parameters calculated in the present study or adopted from the literature.
HD | ST | mV | B − V | ![]() |
E(B − V) | Teff | log g | d | BC a | Mbol | R⋆ |
---|---|---|---|---|---|---|---|---|---|---|---|
number | K | dex | pc | R⊙ | |||||||
34 085 | B8 Iae | 0.13 | − 0.03 | − 0.07 | 0.04 | 11 760 ± 120 | 2.00 ± 0.10 | 264 ± 23 | − 0.83 | − 7.9 ± 0.2 | 72 ± 10 |
38 771 | B0.5 Ia | 2.06 | − 0.18 | − 0.23 | 0.05 | 25 700 ± 260 | 2.70 ± 0.05 | 198 ± 8 | − 2.41 | − 7.0 ± 0.2 | 13 ± 1 |
41 117 | B2 Ia | 4.63 | 0.28 | − 0.18 | 0.42 | 17 940 ± 180 | 2.20 ± 0.05 | 552 ± 85 | − 1.84 | − 7.3 ± 0.4 | 23 ± 3 |
42 087 | B4 Ia | 5.78 | 0.20 | − 0.14 | 0.34 | 15 000 ± 150 | 2.39 ± 0.05 | 2075 ± 1 000s | − 1.46 | − 8.3 ± 1.1 | 55 ± 11 |
47 240 | B1 Ib | 6.15 | 0.15 | − 0.18 | 0.33 | 17 500 ± 180 | 2.40 ± 0.05 | 1598 ± 479 | − 1.78 | − 7.7 ± 0.7 | 30 ± 4 |
52 089 | B1.5 II | 1.50 | − 0.21 | − 0.20 | 0.00 | 21 000 ± 210 | 3.00 ± 0.05 | 124 ± 2 | − 2.20 | − 6.2 ± 0.1 | 11 ± 1 |
52 382 | B1 Ia | 6.50 | 0.19 | − 0.20 | 0.44 | 23 140 ± 230 | 2.47 ± 0.05 | 1301 ± 430s | − 2.05 | − 7.5 ± 0.8 | 21 ± 2 |
53 138 | B3 Ia | 3.02 | − 0.08 | − 0.21 | 0.10 | 18 000 ± 180 | 2.20 ± 0.05 | 847 ± 287 | − 1.66 | − 8.5 ± 0.8 | 46 ± 4 |
58 350 | B5 Ia | 2.45 | − 0.09 | − 0.17 | 0.08 | 15 000 ± 500f | 2.00 ± 0.10f | 609 ± 148 | − 1.24 | − 8.0 ± 0.6 | 54 ± 6 |
64 760 | B0.5 Ib | 4.24 | − 0.14 | − 0.21 | 0.07 | 22 370 ± 220 | 2.50 ± 0.05 | 507 ± 25 | − 2.21 | − 6.7 ± 0.2 | 12 ± 1 |
74 371 | B6 Iab/b | 5.23 | 0.20 | − 0.15 | 0.35 | 13 800 ± 140 | 2.00 ± 0.05 | 1800 ± 360s | − 1.02 | − 8.7 ± 0.5 | 73 ± 10 |
75 149 | B3 Ia | 5.46 | 0.27 | − 0.19 | 0.46 | 15 000 ± 150 | 2.12 ± 0.05 | 1642 ± 330s | − 1.39 | − 8.4 ± 0.7 | 61 ± 13 |
79 186 | B5 Ia | 5.00 | 0.22 | − 0.13 | 0.35 | 15 000 ± 150 | 2.12 ± 0.05 | 1449 ± 609 | − 1.36 | − 8.3 ± 0.9 | 61 ± 7 |
80 077 | B2Ia+e | 7.56 | 1.34 | − 0.16 | 1.50 | 18 000 ± 180 | 2.17 ± 0.05 | 3600 ± 600s | − 1.62 | − 11.6 ± 0.4 | 195 ± 47 |
92 964 | B2.5Ia | 5.38 | 0.27 | − 0.16 | 0.48 | 18 000 ± 180 | 2.19 ± 0.05 | 1851 ± 994 | − 1.66 | − 9.1 ± 1.2 | 70 ± 14 |
99 953 | B1/2 Iab/b | 6.5 | 0.38 | − 0.18 | 0.56 | 18 830 ± 190 | 2.30 ± 0.05 | 1075 ± 427 | − 1.78 | − 7.2 ± 0.9 | 25 ± 3 |
111 973 | B2/3 Ia | 5.94 | 0.24 | − 0.14 | 0.38 | 17 180 ± 170 | 2.18 ± 0.05 | 1660 ± 350s | − 1.46 | − 7.8 ± 0.5 | 46 ± 9 |
115 842 | B0.5 Ia/ab | 6.03 | 0.30 | − 0.23 | 0.60 | 25 830 ± 260 | 2.75 ± 0.05 | 1538 ± 750 | − 2.46 | − 9.2 ± 1.2 | 35 ± 4 |
148 688 | B1 Iaeqp | 5.31 | 0.35 | − 0.20 | 0.54 | 20 650 ± 210 | 2.20 ± 0.05 | 833 ± 229 | − 2.00 | − 8.0 ± 0.7 | 31 ± 4 |
Notes. Values of Teff and log g were derived by fitting the SED, with the exception of those flagged with f. R⋆ is an average of the values obtained from three different approaches (see details in Sect. 3). d is the distance to the star in parsecs derived from HIPPARCOS, with the exception of those data flagged with s. (a)BC: bolometric correction taken from Flower (1996), (f)parameters derived with the code FASTWIND (see details in Sect. 4.1), and (s)distances derived from other methods, see details in the text.
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