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Testing the Breakdown of the Asteroseismic Scaling Relations in Luminous Red Giants

  • Authors: Amanda L. Ash, Marc H. Pinsonneault, Mathieu Vrard, Joel C. Zinn

Amanda L. Ash et al 2025 The Astrophysical Journal 979 .

  • Provider: AAS Journals

Caption: Figure 14.

Frequency spectra for models of different stellar radius and mixing length. Top panel: the y-axis of this figure is the frequency of a given mode on the x-axis. The triangular points are measurements for a model with a radius of 10R. The circular points have a radius of 50R. The point colors indicate the mixing length of the model. Bottom panel: frequency separations between adjacent modes plotted as a function of mode. The dotted lines are models with R* = 10R and the solid lines are with R* = 50R. The colors of the lines show the different mixing lengths and have the same colors as the legend in the top panel. Section 4.4.1 discusses the results of this figure.

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