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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 1.

The red giant branch bump data sample compiled by D. M. Nataf et al. (2013) is compared with Paper I (left) and this paper (right) at 12 Gyr. Paper I models have only scaled-solar composition. The main difference between the two panels is the calibration of fov,env (see Section 2.5 for details).

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