Convective Overshooting in Low-mass Stars Using the k–ω Model
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab262f/pdf
Reference29 articles.
1. The Dependence of Convective Core Overshooting on Stellar Mass: A Semi-empirical Determination Using the Diffusive Approach with Two Different Element Mixtures
2. Significant uncertainties from calibrating overshooting with eclipsing binary systems
3. Proper use of Schwarzschild Ledoux criteria in stellar evolution computations
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2. Grids of Wolf–Rayet Stars Using MESA with the k − ω Model: From 25 to 120 M ⊙ at Z = 0.02;The Astrophysical Journal Supplement Series;2023-09-27
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