Seeds to success: Growing heavy black holes in dense star clusters
Context. The observational dearth of black holes (BHs) with masses between ∼100 and 100 000 M⊙ raises questions about the nature of intermediate-mass black holes (IMBHs). The proposed formation channels for IMBHs include runaway stellar collisions and repeated binary BH (BBH) mergers driven by dynam...
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| Principais autores: | , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
EDP Sciences
2026-04-01
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| Series: | Astronomy & Astrophysics |
| Assuntos: | |
| Acceso en liña: | https://www.aanda.org/articles/aa/full_html/2026/04/aa57230-25/aa57230-25.html |
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