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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 17.

Evolutionary tracks computed with MESA-r21.12.1 (solid gray lines) and MESA-24.08.1 (dashed blue lines) from ZAMS until AGB for models of 3, 4, 5, 6, 7, and 8 M⊙ and different metallicities, Z = 0.014 (left), Z = 0.004 (middle), and Z = 0.0014 (right). Models in the top row do not include overshooting, while in the bottom row overshooting is included.

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