Fig. 9.

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Evolution of the normalised frequencies of non-radial ℓ = 1 modes with radial orders n = [10, 11, 12] for evolutionary tracks of the stellar grid with masses between 1.23 and 1.26 M⊙ as a function of the various age proxies considered for interpolation: τ (left), τscaled (middle), and ρc (right). Different colours are used to represent different stellar masses and different line styles show different radial orders, according to the insets in the middle and right panel, respectively.
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