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Table 1.

Mode frequencies detected in HD 129929 (from A04) and parameters of the best stellar model reproducing this dataset (from D04).

Seismic frequencies [c/d] Asteroseismic model
ν (p1, ℓ0) = 6.590940 M = 9.35 M; log g = 3.905
ν (p1, ℓ1) = 6.966172–6.978305– Teff = 22 392 K; Xc = 0.353
6.990431 Xi = 0.7; Zi = 0.0188
ν (g1, ℓ2) = 6.449590–6.461699 αov = 0.1

Notes. Teff is the effective temperature; logg the surface gravity; Xc, the central H abundance; Xi and Zi the initial H and metal mass fractions; and αov the overshooting parameter.

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