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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 6.

Isochrones at 100 Myr, 1 Gyr, and 10 Gyr from MIST (solid lines) and BaSTI (dashed lines). Darker colors show solar-scaled [α/Fe] = 0 isochrones, while lighter colors show [α/Fe] = +0.4 enhanced isochrones.

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