Published September 30, 2025 | Version v1
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A Spectroscopic Hunt for Post-Red Supergiants in the Large Magellanic Cloud II: Turbulent Line Broadening in the Spectra of LMC Yellow Supergiants

  • 1. ROR icon Carnegie Observatories
  • 2. ROR icon Flatiron Institute
  • 3. ROR icon Carnegie Mellon University
  • 4. ROR icon Howard University

Description

Inlists and run_star_extras.f90 used to produce the YSG MESA models in the paper, "A Spectroscopic Hunt for Post-Red Supergiants in the Large Magellanic Cloud II: Turbulent Line Broadening in the Spectra of LMC Yellow Supergiants." Inlists are adapted from 10.5281/zenodo.6968760, Section 7-Convection/superadiabatic_reduction_models. Uses MESA version r23.05.1.

Values in the inlists that are varied across the set of models shown in the paper are marked with double carets, e.g. <<INITIAL_MASS>>, <<SCALING>>, and <<MIXING_LENGTH>>. 

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Additional details

Related works

Is supplement to
Publication: arXiv:2508.14971 (arXiv)

Dates

Accepted
2025-08-11