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MESA Isochrones and Stellar Tracks (MIST). II. Models with α-enhanced Chemical Composition

  • Authors: Aaron Dotter, Evan B. Bauer, Minjung Park, Charlie Conroy, Antonino P. Milone, Meridith Joyce, Matteo Cantiello

Aaron Dotter et al 2026 The Astrophysical Journal Supplement Series 283 .

  • Provider: AAS Journals

Caption: Figure 2.

MIST isochrones at 10 Myr (upper left), 100 Myr, 1 Gyr, and 10 Gyr (lower right). The left panel shows Z = 0.0017 ([Fe/H] ≈ –1) and the right panel shows Z = 0.016 ([Fe/H] ≈ 0), for both Paper I (red) and this paper (black). In this and subsequent figures, the pre-MS evolution has been omitted from the younger ages for clarity.

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