Intermediate-mass Black Hole Progenitors from Stellar Collisions in Dense Star Clusters
Very massive stars (VMSs) formed via a sequence of stellar collisions in dense star clusters have been proposed as the progenitors of massive black hole seeds. VMSs could indeed collapse to form intermediate-mass black holes, which would then grow by accretion to become the supermassive black holes...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
IOP Publishing
2024-01-01
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| Σειρά: | The Astrophysical Journal |
| Θέματα: | |
| Διαθέσιμο Online: | https://doi.org/10.3847/1538-4357/ad43d6 |
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