Fast-spinning massive black holes from slowly rotating low-metallicity stars: Implications for GW231123
Context. The origin of massive black holes in the early Universe remains uncertain and is still unexplored. Population III (Pop III; zero-metallicity) stars are among the first stellar sources capable of producing such remnants, but their evolution is very sensitive to rotation. Aims. We explore how...
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| Principais autores: | , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
EDP Sciences
2026-07-01
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| coleção: | Astronomy & Astrophysics |
| Assuntos: | |
| Acesso em linha: | https://www.aanda.org/articles/aa/full_html/2026/07/aa60202-26/aa60202-26.html |
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