Table 2
Atmospheric and stellar fundamental parameters for the sample stars.
| ID | Teff (K) | log g | log gF | E(B− V) | B.C. | Mbol | log L∕L⊙ | R∕R⊙ | Mspec∕M⊙ | Sp. type |
|---|---|---|---|---|---|---|---|---|---|---|
| 119 | 8990 ± 450 | 2.16 ± 0.10 | 2.34 ± 0.13 | 0.14 ± 0.03 | −0.08 | −6.37 ± 0.22 | 4.45 ± 0.09 | 69 ± 7 | 25.1 ± 3.3 | A2 Ib * |
| 151 | 10140 ± 510 | 2.32 ± 0.10 | 2.30 ± 0.13 | 0.11 ± 0.03 | −0.30 | −6.15 ± 0.23 | 4.35 ± 0.09 | 49 ± 5 | 18.2 ± 2.5 | A0 Ib * |
| 192 | 10980 ± 550 | 2.23 ± 0.10 | 2.07 ± 0.13 | 0.12 ± 0.03 | −0.46 | −6.30 ± 0.23 | 4.42 ± 0.09 | 45 ± 5 | 12.4 ± 1.7 | B9 Ib |
| 209 | 11840 ± 590 | 2.55 ± 0.10 | 2.26 ± 0.13 | 0.25 ± 0.03 | −0.63 | −6.84 ± 0.24 | 4.63 ± 0.10 | 50 ± 5 | 31.3 ± 4.3 | B9 Ib * |
| 223 | 12500 ± 620 | 2.66 ± 0.10 | 2.27 ± 0.13 | 0.09 ± 0.03 | −0.75 | −6.31 ± 0.24 | 4.42 ± 0.10 | 35 ± 4 | 20.1 ± 2.9 | B8 Ib * |
| 247 | 10370 ± 520 | 2.23 ± 0.10 | 2.17 ± 0.13 | 0.09 ± 0.03 | −0.34 | −5.86 ± 0.23 | 4.25 ± 0.09 | 41 ± 4 | 10.6 ± 1.5 | A0 Ib |
| 462 | 8360 ± 420 | 1.80 ± 0.10 | 2.11 ± 0.13 | 0.51 ± 0.03 | 0.02 | −6.30 ± 0.22 | 4.42 ± 0.09 | 77 ± 8 | 13.6 ± 1.8 | A3 Ib |
| 468 | 12500 ± 630 | 2.66 ± 0.10 | 2.27 ± 0.13 | 0.19 ± 0.03 | −0.75 | −6.11 ± 0.24 | 4.34 ± 0.10 | 32 ± 4 | 16.6 ± 2.3 | B8 Ib * |
| 507 | 9080 ± 450 | 2.17 ± 0.10 | 2.34 ± 0.13 | 0.09 ± 0.03 | −0.09 | −5.10 ± 0.22 | 3.93 ± 0.09 | 38 ± 4 | 7.5 ± 1.0 | A2 II |
| 629 | 8730 ± 440 | 2.12 ± 0.10 | 2.36 ± 0.13 | 0.10 ± 0.03 | −0.03 | −4.82 ± 0.22 | 3.83 ± 0.09 | 36 ± 4 | 6.2 ± 0.8 | A3 II |
| 633 | 9430 ± 470 | 2.30 ± 0.10 | 2.40 ± 0.13 | 0.21 ± 0.03 | −0.16 | −5.54 ± 0.22 | 4.07 ± 0.09 | 41 ± 4 | 12.1 ± 1.6 | A1 II * |
| 641 | 8920 ± 450 | 2.14 ± 0.10 | 2.34 ± 0.13 | 0.15 ± 0.03 | −0.06 | −5.10 ± 0.22 | 3.94 ± 0.09 | 39 ± 4 | 7.6 ± 1.0 | A3 II |
| 645 | 9810 ± 490 | 2.14 ± 0.10 | 2.17 ± 0.13 | 0.22 ± 0.03 | −0.23 | −5.62 ± 0.23 | 4.14 ± 0.09 | 41 ± 4 | 8.4 ± 1.2 | A1 II |
| 709 | 8730 ± 440 | 2.11 ± 0.10 | 2.35 ± 0.13 | 0.09 ± 0.03 | −0.03 | −4.95 ± 0.22 | 3.88 ± 0.09 | 38 ± 4 | 6.7 ± 0.9 | A3 II |
| 759 | 8300 ± 420 | 2.05 ± 0.10 | 2.37 ± 0.13 | 0.15 ± 0.03 | 0.03 | −4.95 ± 0.22 | 3.90 ± 0.09 | 42 ± 4 | 7.2 ± 1.0 | A4 II |
| 200230 | 8300 ± 420 | 2.05 ± 0.10 | 2.37 ± 0.13 | 0.41 ± 0.03 | 0.03 | −6.03 ± 0.22 | 4.31 ± 0.09 | 70 ± 7 | 19.4 ± 2.6 | A4 Ib * |
Notes. ID numbers are taken from Paper I. Spectral types were assigned based on the empirical Teff spectral type and logL∕L⊙ luminosity class relations (see text). An asterisk marks cases with a large mismatch of spectroscopic end evolutionary masses (objects marked in red in Figs. 7 to 9). The results for the corresponding entries should be considered with care; the objects are likely not single stars as discussed in Sect. 4.
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