Table 5
Parameters of our best-fit HDUST model in the BeAtlas grid to explain the joint analysis of our interferometric data: VEGA calibrated and differential data and AMBER differential data.
| M⋆ (M⊙) | Req ∕Rp | i(deg) | PA (deg) | Σ0 (g cm−2) | m | Rp (R⊙) | vrot (km s−1) | vrot/vcrit |
|---|---|---|---|---|---|---|---|---|
| 4.2 | 1.45 | 63.6 | 110 | 0.12 | 3.0 | 3.7 | 368 | 0.96 |
Notes. A part of these parameter values are presented in the last column of Table 4. The polar radius and the stellar rotational velocity are obtained from M⋆ and Req ∕Rp. The linear rotational rate is also shown here (vcrit from Frémat et al. 2005).
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