Many recent observational and theoretical studies suggest that globular clusters (GCs) host compact object populations large enough to play dominant roles in their overall dynamical evolution. Yet direct detection, particularly of black holes and neutron stars, remains rare and limited to special cases, such as when these objects reside in close binaries with bright companions. Here we examine the potential of microlensing detections to further constrain these dark populations. Based on state-of-the-art GC models from the
This content will become publicly available on May 26, 2023
- Publication Date:
- NSF-PAR ID:
- 10356510
- Journal Name:
- The Astrophysical Journal
- Volume:
- 931
- Issue:
- 2
- Page Range or eLocation-ID:
- 84
- ISSN:
- 0004-637X
- Sponsoring Org:
- National Science Foundation
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