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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 2.

Average surface rotational velocities, vrot, as a function of luminosity during crossings of the IS for 3, 5, and 8 M models of different metallicities, Z = 0.014 (top), Z = 0.006 (middle), and Z = 0.002 (bottom). Solid, dashed, and dotted lines correspond to models without MS core overshooting, and with fH = 0.01, and fH = 0.02, respectively. In all models, the initial ZAMS rotation rate is W0 = 0.3.

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