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Table 3

Stellar parameters obtained from the BCD system.

ID ST Teff (K) log g Φ0 (µm) Mv (mag) Mbol (mag) Av (mag)
Hen 3–847(LNA) B6 IV 15 133 ± 1234 3.8 ± 0.10 0.78 ± 0.01 −1.00 ± 0.22 −2.00 ± 0.32 1.30 ± 0.03
Hen 3–847 B6 IV 14905 ± 1071 3.6 ± 0.20 0.78 ± 0.01 −1.25 ± 0.21 −2.17 ± 0.27 1.12 ± 0.03
AS 202(LNA) A1 V: 10408 ± 548 4.3 ± 0.06 0.98 ± 0.03 0.75 ± 0.18 −0.14 ± 0.27 0.78 ± 0.06
AS 202 A0 V: 10335 ± 757 4.5 ± 0.06 0.93 ± 0.03 0.65 ± 0.39(C) 0.33 ± 0.42(F) 0.56 ± 0.06
Hen 3–1398 B0-1 Ia 25 000 ± 1500 2.9 ± 0.11(H) 0.69 ± 0.01 −6.43 ± 0.03(C) −8.62 ± 0.15(F) 2.39 ± 0.03
HD 62623 B9 Ib 11136 ± 318 1.5 ± 0.05(H) 0.88 ± 0.02 −6.25 ± 0.05(C) −6.75 ± 0.09(F) 1.09 ± 0.03
HK Ori B9 V 11940 ± 380 4.1 ± 0.06 0.85 ± 0.02 0.06 ± 0.24 −0.78 ± 0.14 2.05 ± 0.06
CD-24 5721 O8 IV 36 667 ± 3503 3.94 ± 0.09 0.66 ± 0.02 −4.50 ± 0.77 −7.00 ± 0.39 2.29 ± 0.06
HD 85567 B3 III 20 000 ± 1639 3.7 ± 0.16 0.73 ± 0.01 −2.33 ± 0.33 −3.83 ± 0.42 1.12 ± 0.03
CPD-592854 B2 II 21 000 ± 917 2.9 ± 0.08 0.71 ± 0.01 −4.25 ± 0.47 −5.50 ± 0.50 2.02 ± 0.03
MWC 877 B3 Ia: 20 000 ± 2292 2.5 ± 0.20(H) 0.72 ± 0.01 −6.33 ± 0.07(C) -8.22 ± 0.26(F) 4.96 ± 0.03
HD 323 771 B5 V: 17 500 ± 1250 4.3 ± 0.02 0.76 ± 0.01 −1.20 ± 0.19 −2.46 ± 0.34 1.80 ± 0.03
HD 52721 B2 V: 27361 ± 2611: 4.4 ± 0.09: 0.74 ± 0.03: −1.61 ± 0.47: −3.26 ± 1.09: 0.50 ± 0.06
HD 53367 B0 III 32113 ± 4616 2.9 ± 0.16 0.68 ± 0.01 −4.6 ± 1.35 −6.77 ± 0.58 1.30 ± 0.03
HD 58647 B9 IV 12203 ± 600 3.4 ± 0.14 0.87 ± 0.02 −0.50 ± 0.13 −1.25 ± 0.19 0.00 ± 0.06
LHA120-S65 B2 Ib 22 000 ± 1031 2.6 ± 0.08(H) 0.70 ± 0.01 −5.67 ± 0.63 −7.00 ± 0.62 0.19 ± 0.03

Notes. Φ0 is or according to the wavelength range. The symbol “:” indicates extrapolated values. (H)The log g values are estimated from the Teff–log g relationship (log g = 3.98 log Teff − 14.64) found by Haucke et al. (2018).(C)Mv values are estimated from tables given by Cox (2000). (F)Mbol values were calculated using the bolometric correction given by Flower (1996).

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