Image Details

Choose export citation format:

Distinct Stellar Parameter Dependencies of Granulation and Mesogranulation in Red Giants

  • Authors: Anohita Mallick, Jharnesh Verma, Shatanik Bhattacharya, Shravan M Hanasoge

Anohita Mallick et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 2.

Residuals of the predicted versus observed comparison, ﹩\mathrm{ln}({Y}_{{\rm{obs}}}/{Y}_{{\rm{pred}}})﹩, for a2,int, a3,int, b2, b3, as a function of Teff, ﹩\mathrm{log}g﹩, and [Fe/H] were included in the adopted model, for the full sample. The black line shows a running median; the shaded band indicates the ±2σ region. Top row (a)–(d): full sample, color coded by evolutionary phase. Bottom row (e)–(h): the same residuals separated into individual RGB (top), pRC (middle), and sRC (bottom) subpanels, with the running median computed independently within each evolutionary phase

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse