Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins
Ishaan Satish, Kyle Kremer, Fulya Kıroğlu, Daichi Tsuna, Shahed Shayan Aran
astro-ph.HE, astro-ph.GA
Submitted: 2026-07-06
Comments: 14 pages, 10 figures, 1 table. Submitted to MNRAS. Comments welcome!
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Red vs. Blue: How metallicity shapes black hole dynamics and mergers in dense star clusters
- Formation of black holes in the pair-instability mass gap: evolution of a post-collision star
- Machine Learning Methods for Stellar Collisions. I. Predicting Outcomes of SPH Simulations
- Compact Objects in Globular Clusters
- The Origin and Evolution of Multiple Star Systems
- Matching Globular Cluster Models to Observations
- GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- Fates of Rotating Supergiants from Stellar Mergers and the Landscape of Transients upon Core-collapse
- Mass Distribution of Binary Black Hole Mergers from Young and Old Dense Star Clusters
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