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Table 13.
Physical parameters of the asteroseismic best-fit models for the different stars.
| Teff [K] | M* [M⊙] | −log(Menv/M*) | −log(MHe/M*) | −log(MH/M*) | XHe | XO | σrms [s]) | d [pc] | dGaia [pc] |
|---|---|---|---|---|---|---|---|---|---|
| EC 23487-2424: | |||||||||
| 12 300 | 0.68 | 1.7 | 2.0 | 5.0 | 0.7 | 0.9 | 2.95 | 48.96±0.23 | 49.830 |
| BPM 31594: | |||||||||
| 11 500 | 0.57 | 1.6 | 2.0 | 4.5 | 0.5 | 0.9 | 0.84 | 44.27±2.24 | 44.202 |
| BPM 30551: | |||||||||
| 12 100 | 0.72 | 1.7 | 2.0 | 4.5 | 0.9 | 0.9 | 0.84 | 49.17 | 49.743 |
| MCT 0145-2211: | |||||||||
| 11 800 | 0.69 | 1.6 | 2.0 | 5.0 | 0.7 | 0.9 | 1.85 | 44.07±1.42 | 46.157 |
| L 19-2: | |||||||||
| 12 200 | 0.65 | 1.9 | 2.0 | 6.0 | 0.5 | 0.5 | 0.24 | 20.76±0.29 | 20.871 |
| HS 1013+0321: | |||||||||
| 12 000 | 0.59 | 1.6 | 2.0 | 9.0 | 0.6 | 0.7 | 0.33 | 60.43±2.78 | 60.248 |
Notes. We also list the corresponding seismic distances (d), together with the geometric Gaia distances (dGaia).
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