Table 13.
Steps in deriving the seismic distances of the stars.
| PM J22299+3024 | LP 119–10 | |||
|---|---|---|---|---|
| Teff [K] | 11 400 | 10 200 | 11 900 | 11 800 |
| M* [M⊙] | 0.46 | 0.54 | 0.70 | 0.70 |
| log L/L⊙ | −2.453 | −2.742 | −2.652 | −2.667 |
| Mbol [mag] | 10.873 | 11.595 | 11.370 | 11.408 |
| BC [mag] | −0.509 | −0.352 | −0.594 | −0.577 |
| MV [mag] | 11.382 | 11.947 | 11.964 | 11.985 |
| mV [mag] | 16.161 ± 0.01 | 15.294 ± 0.09 | ||
| dseismic [pc] | 90.34 ± 0.42 | 69.62 ± 0.32 | 46.3 ± 1.9 | 45.9 ± 1.9 |
| dGaia [pc] |
 |
45.97 ± 0.09 | ||
Notes. We list the parameters for two models in the case of both stars: the first models belong to the best-fit models not considering the spectroscopic solutions, while the second models belong to models found in the ±3σ vicinity of the spectroscopic Teff and M* values. We also list the Gaia EDR3 geometric distance values for comparison.
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