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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 9.

Slope, α, and intercept, β (see Equation (2)), as a function of metallicity for the PL relation for O24 models on the second and third crossings of the IS. In the bottom panel, linear fits determine the metallicity effect, γ. Open symbols (and fits plotted with dashed line) correspond to the PL relation of fixed slope. In the bottom panel, relations for the second crossing were shifted by 0.1 for better visibility.

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