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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) ReqRp 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 ReqRp. The linear rotational rate is also shown here (vcrit from Frémat et al. 2005).

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