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...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , |
|---|---|
| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
IOP Publishing
2026-01-01
|
| Σειρά: | The Astrophysical Journal |
| Θέματα: | |
| Διαθέσιμο Online: | https://doi.org/10.3847/1538-4357/ae6efb |
| Ετικέτες: |
Δεν υπάρχουν, Καταχωρήστε ετικέτα πρώτοι!
|