The In Situ Growth of Stellar-mass “Light” Seed Black Holes in Nuclear Star Clusters
Remnant black holes (BHs) of massive stars (“light seeds”) are a potential origin for supermassive black holes. We use magnetohydrodynamic simulations to study the formation and growth of light seeds in star-forming giant molecular clouds (GMCs) with masses 10 ^5 –10 ^9 M _⊙ , which evolve for ∼10–3...
I tiakina i:
| Ngā kaituhi matua: | , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2026-01-01
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| Rangatū: | The Astrophysical Journal |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-4357/ae6efb |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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