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Table 21.
Name of the studied stars (Col. 1), the effective temperature and gravity of their asteroseismological or representative models (Cols. 2 and 3), the apparent and absolute Gaia magnitudes (Cols. 4 and 5), and the seismological and astrometric distances (Cols. 6 and 7).
| Name | Teff | log g | mG | MG | ds | dGaia | Distance |
|---|---|---|---|---|---|---|---|
| [K] | [cgs] | [mag] | [mag] | [pc] | [pc] | discrepancy | |
| PG 1351+489 | 25 775 | 8.103 | 16.678 | 10.564 |
 |
 |
4.94 % |
| EC 20058−5234 | 25 467 | 8.062 | 15.756 | 10.518 |
 |
 |
5.38 % |
| EC 04207−4748 | 27 614 | 7.872 | 15.229 | 10.126 |
 |
 |
12.8 % |
| WD J1527−4502 | 25 780 | 7.877 | 15.482 | 10.236 | 111.98 |
 |
16.0 % |
| L 7−44 | 24 690 | 7.921 | 14.737 | 10.354 | 75.26 |
 |
8.0 % |
Notes. Column 8 gives the discrepancy in the distances.
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