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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| Autors principals: | , , , , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
MDPI AG
2024-12-01
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| Col·lecció: | Galaxies |
| Matèries: | |
| Accés en línia: | https://www.mdpi.com/2075-4434/12/6/87 |
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