Table 8
Fundamental physical parameters for the sample of observed stars.
| ID | Name | M V | T eff | log g | [Fe/H] | Spectral | Calibration |
| number | (mag) | (K) | type group | adopted | |||
|
|
|||||||
| ±0.3 | ±0.1 | ||||||
| 1 | VX Cas | 1.5 | 9850 ± 250 | 4.07 ±0.10 | − | A0-A3 | 3 |
| 2 | V594 Cas | −4.1 | 30 500 ± 1000 | 4.05 ± 0.25 | − | B | 2 |
| 3 | PDS 004 | 1.9 | 8030 ± 200 | 4.18 ± 0.10 | −0.10 | A | 1 |
| 4 | XY Per | − | − | − | − | − | − |
| 5 | AB Aur | 0.0 | 8780 ± 200 | 3.64 ± 0.10 | −0.65 | A0-A3 | 3 |
| 6 | HD 31648 | 1.5 | 7870 ± 200 | 4.02 ± 0.10 | −0.19 | A | 1 |
| 9 | HD 35187 | 2.1 | 7490 ± 200 | 4.07 ± 0.10 | −0.29 | A | 1 |
| 10 | HD 287823 | 1.8 | 8740 ± 200 | 4.35 ± 0.10 | −0.18 | A0-A3 | 3 |
| 12 | HD 290409 | 1.7 | 9440 ± 250 | 4.27 ± 0.10 | − | A0-A3 | 3 |
| 13 | HD 290500 | 3.6 | 7700 ± 200 | >4.50 | −0.46 | A | 1 |
| 14 | V1409 Ori | 0.8 | 7820 ± 200 | 4.19 ± 0.10 | −0.02 | A | 1 |
| 15 | HD 36112 | 2.1 | 7770 ± 200 | 4.16 ± 0.10 | 0.02 | A | 1 |
| 16 | V1410 Ori | 1.4 | 8140 ± 200 | 4.06 ± 0.10 | −0.02 | A | 1 |
| 17 | HD 36408 | −1.6 | 11 950 ± 350 | 3.22 ± 0.15 | − | B | 2 |
| 18 | V1271 Ori | −0.1 | 9310 ± 250 | 3.56 ± 0.10 | − | A0-A3 | 3 |
| 19 | V380 Ori | – | − | − | − | − | − |
| 20 | HD 290770 | −1.1 | 11 300 ± 350 | 3.41 ± 0.15 | − | B | 2 |
| 21 | BF Ori | 0.1 | 8600 ± 200 | 3.67 ± 0.10 | 0.35 | A0-A3 | 1 |
| 22 | HD 37357 | 1.2 | 8790 ± 200 | 4.09 ± 0.10 | −0.25 | A0-A3 | 3 |
| 23 | V1247 Ori | 0.7 | 7060 ± 200 | 3.64 ± 0.10 | 0.55 | F | 1 |
| 24 | V1788 Ori | 1.4 | 8470 ± 200 | 4.16 ± 0.10 | −0.22 | A0-A3 | 1 |
| 25 | RR Tau | − | − | − | − | − | − |
| 26 | V350 Ori | 2.1 | 8500 ± 200 | 3.74 ± 0.10 | 0.91 | A0-A3 | 1 |
| 27 | HD 37806 | –1.6 | 11 500 ± 350 | 3.18 ± 0.15 | − | B | 2 |
| 28 | HD 38120 | −0.9 | 10 700 ± 250 | 2.66 ± 0.10 | − | B | 3 |
| 30 | HD 249879 | −0.3 | 11 350 ± 350 | 3.68 ± 0.15 | − | B | 2 |
| 31 | V791 Mon | −3.2 | 25 600 ± 1000 | 4.07 ± 0.25 | − | B | 2 |
| 32 | HD 250550 | −3.0 | 12 800 ± 350 | 2.81 ± 0.15 | − | B | 2 |
| 33 | AE Lep | 1.9 | 8050 ± 200 | 4.18 ± 0.10 | −0.84 | A | 1 |
| 34 | PDS 126 | 2.5 | 8650 ± 200 | 4.50 ± 0.10 | 0.18 | A0-A3 | 1 |
| 35 | HD 50083 | − | − | − | − | − | − |
| 36 | HD 52721 | −4.7 | 33 800 ± 1500 | 4.21 ± 0.25 | − | B | 2 |
| 37 | HT Cma | 0.6 | 10 560 ± 250 | 3.61 ± 0.10 | − | B | 3 |
| 38 | HU Cma | −1.3 | 16 000 ± 500 | 4.15 ± 0.15 | − | B | 2 |
| 39 | HD 53367 | − | − | − | − | − | − |
| 40 | PDS 241 | − | − | − | − | − | − |
| 41 | HD 141569 | 0.4 | 9220 ± 250 | 3.93 ± 0.10 | −0.64 | A0-A3 | 3 |
| 42 | VV Ser | −5.5 | 12 150 ± 350 | 2.06 ± 0.15 | − | B | 2 |
| 43 | V431 Sct | − | − | − | − | − | − |
| 44 | HD 174571 | −2.4 | 22 700 ± 1000 | 4.13 ± 0.25 | − | B | 2 |
| 45 | HD 179218 | −0.3 | 8930 ± 200 | 3.55 ± 0.10 | −0.72 | A0-A3 | 3 |
| 46 | WW Vul | 1.2 | 7770 ± 200 | 3.87 ± 0.10 | 0.22 | A | 1 |
| 47 | PX Vul | 4.5 | 6120 ± 150 | >4.50 | −1.18 | F | 1 |
| 48 | PDS 581 | − | − | − | − | − | − |
| 49 | HD 190073 | − | − | − | − | − | − |
| 50 | V1685 Cyg | − | − | − | − | − | − |
| 51 | HD 200775 | − | − | − | − | − | − |
| 52 | HD 203024 | 1.8 | 7820 ± 200 | 4.09 ± 0.10 | −0.63 | A | 1 |
| 53 | BD +65.1637 | −3.6 | 27 200 ± 1000 | 3.99 ± 0.25 | − | B | 2 |
| 54 | V1578 Cyg | −1.0 | 10 830 ± 250 | 2.66 ± 0.10 | − | B | 2 |
| 55 | BH Cep | 3.6 | 6750 ± 150 | 4.50 ± 0.10 | 0.36 | F | 1 |
| 56 | SV Cep | 1.5 | 8830 ± 200 | 4.39 ± 0.10 | −0.63 | A0-A3 | 3 |
| 57 | V1080 Tau | − | − | − | − | − | − |
| 58 | CO Ori | − | − | − | − | − | − |
| 59 | V1650 Ori | 3.6 | 6170 ± 150 | 4.25 ± 0.10 | 0.23 | F | 1 |
| 60 | RY Ori | 7.1 | 5810 ± 150 | >4.50 | 2.72 | F | 1 |
| 61 | HD 36910 | 2.8 | 7230 ± 200 | 4.11 ± 0.10 | 1.10 | F | 1 |
| 62 | HD 53240 | −3.1 | 11 100 ± 350 | 2.57 ± 0.15 | − | B | 2 |
| 63 | HD 261387 | 1.6 | 8400 ± 200 | 4.23 ± 0.10 | −0.10 | A0-A3 | 1 |
Notes. Calibrations adopted: 1: NEMO-2004 CGM (Nendwich et al. 2004; Heiter et al. 2002). Late group, the parameters (b – y)0 and c0 are used here as temperature and luminosity indicators, respectively. 2: Napiwotzki et al. (1993). Early group, the parameters c0 and β are used as temperature and luminosity indicators, respectively. 3: Moon & Dworetsky (1985). Intermediate group, the parameters a0yr∗ together with a log g correction (Napiwotzki et al. 1993) are used for this group.
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