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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 1.

Location of the F-mode IS determined for (panel (a)) different crossing numbers, (panel (b)) different metallicities, (panel (c)) different parameter sets describing convection–pulsation coupling, and (panel (d)), models with and without convective core overshoot. In all panels evolutionary tracks of the O24 set and 2, 3, 4, 6, and 8 M⊙ are plotted for reference.

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