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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 8.

Comparison of the observed and model PL relations expressed in terms of the Wesenheit index, WVI, for the LMC (left) and SMC (right). OGLE data are compared to Z = 0.006 models (LMC) and Z = 0.003 (SMC) without overshooting (O00, top) and including overshooting (O24, bottom). Model relations are shown for the blue and red edges, and midline of the IS, with blue, red, and green colors, respectively. Relations for different crossings are plotted with different line styles, as indicated in the legend (relations for the second and third crossings largely overlap).

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