Predicting stellar collision outcomes for main sequence stars
Context. Stellar collisions in dense galactic nuclei could play an important role in fueling supermassive black holes (SMBHs) and shaping their environments. The gas released during these collisions might contribute to SMBH accretion, influencing phenomena such as active galactic nuclei (AGNs) and t...
Збережено в:
| Автор: | |
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| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
EDP Sciences
2026-02-01
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| Серія: | Astronomy & Astrophysics |
| Предмети: | |
| Онлайн доступ: | https://www.aanda.org/articles/aa/full_html/2026/02/aa57238-25/aa57238-25.html |
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