Super-Eddington accretion in protogalactic cores
The presence of massive black holes (BHs) exceeding 109 M⊙ already at redshift z > 6 challenges standard models of BH growth. Super-Eddington (SE) accretion has emerged as a promising mechanism to solve this issue, yet its impact on early BH evolution in tailored numerical experiments remains largel...
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| Asıl Yazarlar: | , , , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
EDP Sciences
2026-04-01
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| Seri Bilgileri: | Astronomy & Astrophysics |
| Konular: | |
| Online Erişim: | https://www.aanda.org/articles/aa/full_html/2026/04/aa57006-25/aa57006-25.html |
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