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Asteroseismology of red giant stars: The potential of dipole modes

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Figure

Figure 1. Left panela function of the total mass for models without (solid lines) and with (dash-dotted line) overshooting, and chemicalcompositionthe exhaustion of helium at the center for masses lower and larger thanthe RGB models with the same radius as
Figure 2. Evolutionary track of a 1.5 M101.7the red giant phase, RGB and central He-burning.Dots and labels mark location of models discussedin the text and in Figs.is the model withdensity contrast (before the He-shell development, with⊙ star in 3, 4 and
Figure 3. Panels A–F: Oscillations spectra for models A–F in Fig.the frequency domain of solar like oscillations
Figure 4. Expected echelle diagram for the oscillation spectra of models A–F in Fig. 2
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