Open Access
Table 1.
Stellar parameters adopted for our models.
| ID | Teff |
 |
log g | M | R(1) | δ |
|---|---|---|---|---|---|---|
| [K] | [M⊙] | [R⊙] | ||||
| A1 | 7000 | 8.0 | 0.5 | 5395 | 6723 | 1.352 |
| A2 | 7000 | 9.0 | 0.5 | 53 956 | 21 506 | 1.052 |
| A3 | 10 000 | 8.0 | 0.8 | 2585 | 3340 | 1.452 |
| A4 | 10 000 | 9.0 | 0.8 | 25 848 | 10 580 | 1.062 |
| B1 | 137 000 | 8.4 | 5.5 | 10 000 | 30 | 0 |
| B2 | 43 000 | 8.4 | 3.5 | 10 000 | 301 | 0.5 |
| B3 | 13 600 | 8.4 | 1.5 | 10 000 | 3006 | 1 |
| C1 | 77 000 | 7.4 | 4.5 | 1000 | 30 | 0 |
| C2 | 43 000 | 7.4 | 3.5 | 1000 | 95 | 0.5 |
| C3 | 24 000 | 7.4 | 2.5 | 1000 | 305 | 1 |
Notes. For series A models, Teff is adopted. Teff of models for the B and C series is derived from the prescriptions of Gieles et al. (2018a). See text for details. (1)R is the stellar radius at an optical depth equal to 2/3. 2δ is calculated from mass and radius (see text).
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