Assessment of Critical Convection and Associated Rotation States in Models of Sun-like Stars Including a Stable Layer
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab7fa6/pdf
Reference39 articles.
1. Theoretical seismology in 3D: nonlinear simulations of internal gravity waves in solar-like stars
2. Characterizing the propagation of gravity waves in 3D nonlinear simulations of solar-like stars
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5. MODELING THE DYNAMICAL COUPLING OF SOLAR CONVECTION WITH THE RADIATIVE INTERIOR
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1. Effect of Rotation on Wave Mixing in Intermediate-mass Stars;The Astrophysical Journal;2024-07-23
2. Magnetochronology of solar-type star dynamos;Astronomy & Astrophysics;2024-04
3. Stochastic excitation of internal gravity waves in rotating late F-type stars: A 3D simulation approach;Astronomy & Astrophysics;2022-11
4. Powering Stellar Magnetism: Energy Transfers in Cyclic Dynamos of Sun-like Stars;The Astrophysical Journal;2022-02-01
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