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Table 2.
Parameters of the ESTER Vega model of Espinosa Lara & Rieutord (2013) that match the observational constraints (interferometric and spectroscopic) derived by Monnier et al. (2012).
| M (M⊙) | 2.374 |
| Rp (R⊙) | 2.420 |
| Re (R⊙) | 2.728 |
| ϵ | 0.113 |
| L (L⊙) | 48.0 |
| Teffp (K) | 10 070 |
| Teffe (K) | 8970 |
| log gp | 4.046 |
| log ge | 3.815 |
| veq (km s−1) | 205 |
| Ωe (10−4 rad s−1) | 1.082 |
| Ωc (10−4 rad s−1) | 3.067 |
Notes. For that model, ω = 0.504. Indices e and p refer to equatorial and polar values, respectively.
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