How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman–Werner Background
Observing the first generation of Population III (Pop III) stars is one of the most demanding challenges in astronomy. Indeed, Pop III stars are expected to predominantly form within faint minihalos at early times with a top-heavy initial mass function, resulting in efficient metal enrichment and a...
Shranjeno v:
| Principais autores: | , , , , , , |
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| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
IOP Publishing
2026-01-01
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| Serija: | The Astrophysical Journal |
| Teme: | |
| Online dostop: | https://doi.org/10.3847/1538-4357/ae809e |
| Oznake: |
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