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Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting

  • Authors: Radoslaw Smolec, Oliwia Ziółkowska, Rajeev Singh Rathour, Vincent Hocdé, Piotr Wielgórski

Radoslaw Smolec et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 5.

The effects of mass loss (η = 0.6) on evolutionary tracks of high (Z = 0.014, left panel) intermediate (Z = 0.004, middle panel), and low (Z = 0.0014, right panel) metallicity. The models include overshooting both from the MS core and envelope (O24_ML6 models). Tracks are color coded according to a fraction of mass lost, ΔM. Tracks without mass loss (O24) are plotted with dashed black lines for reference.

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