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...
Enregistré dans:
| Auteurs principaux: | , |
|---|---|
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
IOP Publishing
2024-01-01
|
| Collection: | The Astrophysical Journal |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.3847/1538-4357/ad5723 |
| Tags: |
Pas de tags, Soyez le premier à ajouter un tag!
|