Table 3
Sensitivity of the stellar characteristics to the model parameters.
| αov | 0 | 0.1 | 0.2 |
|
|
|||
| M/M⊙ | 3.9–4.2 | 3.6–4.0 | 3.6–4.0 |
| R/R⊙ | 29.5–30.5 | 28–30 | 27.5–30 |
| αCGM | 0.6 | 0.7 | 0.8 |
|
|
|||
| M/M⊙ | 4.4–4.8 | 3.6–4.1 | 3.3–4.0 |
| R/R⊙ | 31–32 | 29–30 | 27–29 |
| [Fe/H] | 0 | –0.18 |
|
|
||
| M/M⊙ | 3.6–4.0 | 3.5–3.7 |
| R/R⊙ | 27.5–31 | 27–28 |
Notes. The estimates presented correspond to the models giving the lowest χ2. These estimates are drawn from the results of Fig. 9 for the mass and from similar results not shown for the radius. They do not aim at a quantitative comparison but at an overall view only.
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