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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 18.

The effect of 14N(p, γ)15O reaction rate (the default JINA REACLIB, solid gray lines vs. the NACRE rate, dashed green lines) across metallicity (Z = 0.014, Z = 0.004, and Z = 0.0014, in the left, middle, and right columns, respectively) and overshooting (no overshoot and core and envelope overshoot enabled, in the top and bottom rows, respectively) scenarios. Fiducial hot IS strip is overplotted for reference.

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