Black hole mergers in compact star clusters and massive black hole formation beyond the mass gap
We present direct N-body simulations, carried out with nbody6+ + gpu, of young and compact low-metallicity (Z = 0.0002) star clusters with 1.1 × 105 stars, a velocity dispersion of ∼15 km, s-1, a half-mass radius Rh = 0.6 pc, and a binary fraction of 10per,cent including updated evolution models for...
| Main Authors: | , , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Oxford University Press
2022
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| Subjects: | |
| Online Access: | View Fulltext in Publisher |