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The YREC Stellar Evolution Code: Public Data Release

  • Authors: Marc H. Pinsonneault, Jennifer L. van Saders, Lyra Cao, Jamie Tayar, Franck Delahaye, Leslie M. Morales, Rachel A. Patton, Matthew C. Rendina, Joel C. Zinn, Zachary R. Claytor, Amanda L. Ash, Susan Byrom, Kaili Cao, Vincent A. Smedile

Marc H. Pinsonneault et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 15.

Rotating models compared against a select sample of open cluster rotation sequences from J. L. Curtis et al. (2020) and D. Gruner et al. (2023). Solid curves (top panel) denote models that include the full treatment of microscopic diffusion, internal AM transport, and wind braking. Dashed curves (bottom panel) represent strongly magnetically coupled models, where solid-body rotation is enforced at all times.

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