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Table 5

Parameters and uncertainties estimated from a Levenberg-Marquardt fit of our model to the VLTI/AMBER φdiff observed on studied stars, and compared with values found in the literature.

New studied stars

Parameters Altair δ Aquilae Fomalhaut

Comparison of best fit values those from literature

Best-fit parameter In this paper In the literature In this paper In the literature In this paper In the literature

Equatorial radius Req 2.0 ± 0.2 R 2.029 ± 0.007 Ra 2.2 ± 0.3 R Rmean = 2.04 R b 1.8 ± 0.2 R Rmean = 1.8 R f
Equatorial rotation velocity Veq 269 ± 14 km s-1 285.8 ± 12 km s-1a 75 ± 23 km s-1 Veqsini = 68.4 km s-1e to 89 km s-1c 93 ± 7 km s-1 93 km s-1d
Rotation-axis inclination angle i 57.3 ± 5.6° 57.2 ± 1.9°a 81 ± 13° 90 ± 9°
Rotation-axis position angle PArot 65.5 ± 5.5° 61.8 ± 0.8°a 101.2 ± 13.6° 65.6 ± 4.7° 65 ± 3°d

χ 2 1.8775 1.3297 0.44132

Fixed parameter Value

Distance d 5.14 pca 15.5 pcb 7.66 pcf
Mass M 1.791 Ma 1.65 Mb 2 Mf
Surface mean effective temperature 7700 Ka 7119 Ke 8760 Kf
Gravity-darkening coefficient β 0.19a 0.20 0.20

Derived parameter Value

Equatorial angular diameter eq 3.69 ± 0.36 mas 1.27 ± 0.17 mas 2.19 ± 0.24 mas
Equatorial-to-polar radii Req/Rp 1.22 ± 0.12 1.02 ± 0.14 1.02 ± 0.11
Veqsini 226 ± 12 km s-1 74 ± 23 km s-1 93 ± 7 km s-1
V eq / V crit 0.74 ± 0.04 0.26 ± 0.08 0.25 ± 0.02
Polar effective temperature Tpol 8912 ± 234 K 7233 ± 510 K 8909 ± 342 K
Equatorial effective temperature Teq 7372 ± 937 K 7123 ± 1107 K 8764 ± 1024 K
Luminosity log L/L 1.025 ± 0.028 1.002 ± 0.037 1.192 ± 0.038

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