Hydrodynamics and Nucleosynthesis of Jet-driven Supernovae. I. Parameter Study of the Dependence on Jet Energetics

Rotating massive stars with initial progenitor masses M _prog ∼ 25–140 M _⊙ can leave rapidly rotating black holes to become collapsars. The black holes and the surrounding accretion disks may develop powerful jets by magnetohydrodynamics instabilities. The propagation of the jet in the stellar enve...

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Номзүйн дэлгэрэнгүй

Үндсэн зохиолчид:	Shing-Chi Leung, Ken’ichi Nomoto, Tomoharu Suzuki
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	IOP Publishing 2023-01-01
Цуврал:	The Astrophysical Journal
Нөхцлүүд:	Explosive nucleosynthesis Supernovae Hypernovae Hydrodynamical simulations Chemical abundances Relativistic jets
Онлайн хандалт:	https://doi.org/10.3847/1538-4357/acbdf5
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!