Asteroseismology of evolved stars with EGGMiMoSA - I. Theoretical mixed-mode patterns from the subgiant to the RGB phase

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Fig. 9.

Variation of Δπ₁ with Δν₀ for different masses, depicted by the colours. The dashed lines correspond to the asymptotic value. The dotted vertical lines correspond to the transition between subgiant and red-giant phases.

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