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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 6.

Luminosity as a function of temperature for the solar metallicity models. The solid black and red lines show the locations of ZAMS and TAMS, respectively. We show a comparison of evolutionary tracks from YREC (solid), PARSEC (dashed), and MIST (dashed–dotted) model grids for solar metallicity and Z = 0.017 for PARSEC. Tracks are shown for masses of 0.3, 1.0, 3.0, and 9.0 M⊙, as available in each model library. The 1.0, 3.0, and 9.0 M⊙ tracks are ended at He core ignition.

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