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Stellar Evolution and Convection in 3D Hydrodynamic Simulations of a Complete Burning Phase

Our understanding of stellar evolution and nucleosynthesis is limited by the uncertainties coming from the complex multi-dimensional processes in stellar interiors, such as convection and nuclear burning. Three-dimensional stellar models can improve this knowledge by studying multi-D processes, but...

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Principais autores: Federico Rizzuti, Raphael Hirschi, Vishnu Varma, William David Arnett, Cyril Georgy, Casey Meakin, Miroslav Mocák, Alexander StJ. Murphy, Thomas Rauscher
Formato: Artigo
Idioma:Inglês
Publicado em: MDPI AG 2024-12-01
coleção:Galaxies
Assuntos:
convection
hydrodynamics
nuclear reactions, nucleosynthesis, abundances
stars: evolution
stars: interiors
stars: massive
Acesso em linha:https://www.mdpi.com/2075-4434/12/6/87
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