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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 13.

Sound speed vs. acoustic radius for models with different radii and mixing lengths. The solid and dashed lines refer to stars with 50R and 10R, respectively. The different colored lines indicate the different mixing lengths in the model. The bottom panel shows the fractional difference in the sound-speed profiles compared to the sound-speed profile for a mixing length of 1.7 as a function of the acoustic radius for the different-radii stars. Refer to Section 4.4.1 for plot interpretation.

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