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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 4.

MIST isochrones at 10 Myr, 100 Myr, 1 Gyr, and 10 Gyr. The red line is the α-enhanced model with [Fe/H] = −0.5 (left) or −0.25 (right) while the blue line is made from a scaled-solar composition but interpolated to the same total Z as the red curve in each panel. For comparison, the gray lines are scaled-solar models with the same [Fe/H] as the red lines.

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