The Observed Rate of Binary Black Hole Mergers can be Entirely Explained by Globular Clusters
- Award ID(s):
- 2009916
- NSF-PAR ID:
- 10292537
- Date Published:
- Journal Name:
- Research Notes of the AAS
- Volume:
- 5
- Issue:
- 1
- ISSN:
- 2515-5172
- Page Range / eLocation ID:
- 19
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
More Like this
No document suggestions found