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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| Автори: | , , , |
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| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
EDP Sciences
2026-04-01
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| Серія: | Astronomy & Astrophysics |
| Предмети: | |
| Онлайн доступ: | https://www.aanda.org/articles/aa/full_html/2026/04/aa58114-25/aa58114-25.html |
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