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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 4.

Component analysis of the scaling relations using clusters in the M*vsR* plane. The different colors indicate the different samples within the cluster. The colored dotted lines are the weighted mean masses of a particular sample within a cluster. Left: masses computed using the full scaling relation with a constant ﹩{F}_{{\nu }_{{\max }}}﹩value for RGB and RC stars. Middle: masses using the ﹩{\nu }_{{\rm{\max }}}﹩-only scaling relation with a constant ﹩{\nu }_{{\rm{\max }}}﹩ for RGB and RC stars and parallax-corrected Gaia radii. Right: masses using the Δν-only scaling relation with parallax-corrected Gaia radii. See Section 3.2.1 for discussion of this figure.

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