ASURA-FDPS-ML: Star-by-star Galaxy Simulations Accelerated by Surrogate Modeling for Supernova Feedback

We introduce new high-resolution galaxy simulations accelerated by a surrogate model that reduces the computation cost by approximately 75%. Massive stars with a zero-age main-sequence mass of more than about 10 M _⊙ explode as core-collapse supernovae (CCSNe), which play a critical role in galaxy f...

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Autors principals:	Keiya Hirashima, Kana Moriwaki, Michiko S. Fujii, Yutaka Hirai, Takayuki R. Saitoh, Junichiro Makino, Ulrich P. Steinwandel, Shirley Ho
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Galactic winds Galaxy evolution Hydrodynamical simulations Stellar feedback Interstellar medium
Accés en línia:	https://doi.org/10.3847/1538-4357/add689
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