Fig. 6.
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Stellar structure and oscillations of a 1.0 M⊙ star from the single-star model (red) and a mass-donor model (black). Left panels: Profiles of the Lamb frequency, log Sl = 1 (solid lines: left y axis), and the hydrogen mass fraction, X (dashed lines: right y axis), in the mass co-ordinates (x axis). Middle panels: Corresponding acoustic-model frequency separation ratios, r01, r10, and r02 (squares, triangles, and circles), between small and large frequency separations, respectively, which are calculated with Equations (7). Right panels: Normalized large-frequency separation (Δνl/⟨Δνl⟩) (l = 0, 1, 2, corresponding to squares, triangles, and circles) as a function of radial order (n).
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