Table 1.
Mass, effective temperature, luminosity, and radius characteristic of the H-burning limit (t = 10 Gyr) with the Saumon et al. (1995), Chabrier et al. (2019) and Chabrier & Debras (2021) EOSs, all calculated with the ATMO atmosphere models.
| EOS | MHBMM/M⊙ | TeffHBL [K] | log(L/L⊙)HBL | RHBL/R⊙ |
|---|---|---|---|---|
| SCvH+COND (Baraffe et al. 2003) | 0.072 | 1560 | −4.47 | 0.081 |
| SCvH+ATMO | 0.073 | 1807 | −4.14 | 0.087 |
| CMS’19+ATMO (Phillips et al. 2020) | 0.074 | 1800 | −4.16 | 0.085 |
| CD’21+ATMO (present) | 0.075 | 1800 | −4.19 | 0.083 |
Notes. For the sake of comparison, the results with the COND atmosphere models are also presented.
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