Glitches in solar-like oscillating F-type stars - Theoretical signature of the base of the convective envelope on the ratios r010

Open Access

Fig. 9.

Impact of the μ-gradient and of the smoothness of the temperature gradient on the r₀₁₀ ratios. Left: temperature gradients of model B2 (orange), B3 (blue), and B4 (green) for the top panel, and A5 (orange), A6 (blue), and A7 (green) for the bottom panel as a function of the acoustic radius at X_c = 0.10. Right: corresponding r₀₁₀ ratios as a function of the frequency.

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