Quasi-stars as a Means of Rapid Black Hole Growth in the Early Universe
JWST observations demonstrate that supermassive black holes (SMBHs) exist by redshifts z ≳ 10, providing further evidence for “direct collapse” black hole (BH) formation, whereby massive (∼10 ^3–5 M _⊙ ) SMBH seeds are generated within a few million years as a byproduct of the rapid inflow of gas in...
Gardado en:
| Principais autores: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
IOP Publishing
2024-01-01
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| Series: | The Astrophysical Journal |
| Assuntos: | |
| Acceso en liña: | https://doi.org/10.3847/1538-4357/ad5723 |
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