Radiation magnetohydrodynamics simulations of Population III star formation during the epoch of reionization

Cosmological simulations find that pockets of star-forming gas could remain pristine up until the epoch of reionization (EoR) due to the inhomogeneous nature of metal mixing and enrichment in the early Universe. Such pristine clouds could have formed Population III stars, which could have distinct p...

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Номзүйн дэлгэрэнгүй

Үндсэн зохиолчид:	van Veenen Lisanne, Sharda Piyush, Viti Serena, Menon Shyam H.
Формат:	Artigo
Хэл сонгох:	Inglês
Хэвлэсэн:	EDP Sciences 2026-04-01
Цуврал:	Astronomy & Astrophysics
Нөхцлүүд:	magnetohydrodynamics (mhd) radiation mechanisms: general stars: formation stars: massive stars: population iii cosmic background radiation
Онлайн хандалт:	https://www.aanda.org/articles/aa/full_html/2026/04/aa58114-25/aa58114-25.html
Шошгууд:	Шошго нэмэх Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!