Modelling Time-dependent Convective Penetration in 1D Stellar Evolution

Modelling Time-dependent Convective Penetration in 1D Stellar Evolution

One-dimensional stellar evolution calculations produce uncertain predictions for quantities like the age, core mass, core compactness, and nucleosynthetic yields; a key source of uncertainty is the modeling of interfaces between regions that are convectively stable and those that are not. Theoretica...

Deskribapen osoa

Xehetasun bibliografikoak
Egile Nagusiak: Cole Johnston, Mathias Michielsen, Evan H. Anders, Mathieu Renzo, Matteo Cantiello, P. Marchant, Jared A. Goldberg, Richard H. D. Townsend, Gautham Sabhahit, Adam S. Jermyn
Formatua: Artikulua
Hizkuntza:English
Argitaratua: IOP Publishing 2024-01-01
Saila:The Astrophysical Journal
Gaiak:
Stellar evolution
Stellar convective zones
Stellar structures
Stellar interiors
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ad2343

Internet

https://doi.org/10.3847/1538-4357/ad2343

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