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Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops

  • Authors: Radoslaw Smolec, Rajeev Singh Rathour, Vincent Hocdé

Radoslaw Smolec et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 8.

P–Age relations for O24_ML4h_RA models (fH = 0.02, fenv = 0.04, ηR = 0.4) without rotation (top panels) and with the highest initial rotation rate of W0 = 0.65 (bottom panels), for MW, LMC, and SMC metallicities (Z = 0.014, 0.006, and 0.002 in the left, middle, and right panels, respectively). Relations are plotted for each crossing; the upper and lower envelopes of the bands correspond to the red and blue edges of the IS, respectively.

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