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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 9.

Evolutionary tracks for 3, 4, 5, and 7 M⊙ from MIST (J. Choi et al. 2016). Model metallicities, [Fe/H], are +0.0, −0.25, and −0.75 from left to right. Solid lines correspond to models without rotation, while models plotted with blue dashed lines correspond to an initial rotation rate at ZAMS of W0 = 0.4.

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