Table 4
Observational data and results of modeling
| Mazzei & Barbaro (2011) | Wegner (2002) | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Name | Sp. | E(B − V) | CCM RV | RV |  |
Sp. | E(B − V) | RV | λmax | λmax Reference | |
| (mag) | (mag) | (Å) | |||||||||
| HD 54439 | B2III | 0.28 | 2.13 ± 0.41 | 1.98 | 0.82 | B1V | 0.28 | 2.88 | 4859 ± 129 | This work (VLT) | |
| HD 73420 | B2II/III | 0.37 | 2.47 ± 0.32 | 2.24 | 2.3 | … | … | … | 5465 ± 175 | This work (VLT) | |
| HD 78785 | B2II | 0.76 | 2.55 ± 0.17 | 2.29 | 3.4 | B2II | 0.67 | 3.08 | 5732 ± 8.2 | This work (VLT) | |
| HD 96042 | O9.5V | 0.48 | 1.97 ± 0.24 | 1.87 | 5.2 | B1V | 0.41 | 3.05 | 5109 ± 124 | This work (VLT) | |
| HD 141318 | B2II | 0.30 | 1.95 ± 0.18 | 1.77 | 3.6 | … | … | … | 5719 ± 17 | This work (VLT) | |
| HD 152245 | B0III | 0.42 | 2.25 ± 0.29 | 2.02 | 3.7 | B0Ib | 0.31 | 2.95 | 6169 ± 33 | This work (VLT) | |
| HD 152853 | B2II/III | 0.37 | 2.50 ± 0.33 | 2.19 | 0.91 | … | … | … | 5584 ± 46 | This work (VLT) | |
| BD+23 3762 | B0.5III | 1.05 | 2.47 ± 0.12 | 2.15 | 1.3 | … | … | … | 4965 ± 61 | This work (CAHA) | |
| BD+45 3341 | B1II | 0.74 | 2.46 ± 0.17 | 2.22 | 2.84 | … | … | … | 5166 ± 31 | This work (CAHA) | |
| HD 28446 | B0III | 0.46 | 2.46 ± 0.26 | 2.20 | 1.6 | … | … | … | 4865 ± 76 | This work (CAHA) | |
| HD 194092 | B0.5III | 0.41 | 2.50 ± 0.30 | 2.18 | 3.6 | … | … | … | 5884 ± 107 | This work (Asiago) | |
| HD 14357 | B2II | 0.56 | 2.31 ± 0.21 | 2.12 | 1.4 | B1.5II | 0.49 | 2.88 | 4942 ± 31 | This work (Asiago) | |
| HD 226868 | B0Ib | 1.08 | 3.20 ± 0.14 | 2.78 | 3.3 | B0Ib | 1.03 | 3.32 | 4424.6 ± 262.4 | (This work, HPOL) | |
| HD 218323 | B0III | 0.90 | 2.55 ± 0.15 | 2.30 | 2.6 | … | … | … | 4836.7 ± 128.2 | (This work, HPOL) | |
| HD 217035 | B0V | 0.76 | 2.77 ± 0.18 | 2.44 | 0.5 | … | … | … | 5309.3 ± 125.9 | (This work, HPOL) | |
| HD 2619 | B0.5III | 0.85 | 2.55 ± 0.15 | 2.34 | 3.5 | … | … | … | 4900 ± 100 | Coyne et al. (1974) | |
| HD 37061 | B1V | 0.52 | 4.50 ± 0.38 | 3.82 | 0.8 | B0.5V | 0.47 | 4.14 | 6300 ± 400 | Coyne et al. (1974) | |
| HD 168021 | B0Ib | 0.55 | 3.15 ± 0.27 | 2.74 | 0.02 | … | … | … | 5900 ± 100 | Serkowski et al. (1975) | |
Notes. Spectral type (Sp.), E(B − V) and CCM RV, RV, and RSi are taken from Tables 1 and 4 of Mazzei & Barbaro (2011). The Sp. and E(B − V) values in Mazzei & Barbaro (2011) are taken from Savage et al. (1985). CCM RV is determined by fitting the IR observations with the CCM extinction curve, while RV is determined from the best-fit of WD01 model to all observed data (see Mazzei & Barbaro 2011). For comparison, cols. 7-9 report Sp., E(B − V), and RV values for seven common stars from Wegner (2002).
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