Formation of Black Hole-White Dwarf X-ray Binaries in Globular Clusters

arXiv:2606.25030 · astro-ph.HE · Submitted 2026-06-23 · Read on arXiv

William Y. W. Yang, Kyle Kremer, James C. Lombardi,, Kristen C. Dage

astro-ph.HE

Submitted: 2026-06-23

Comments: 19 pages, 9 figures, 1 table. Submitted to ApJ. Comments are welcome

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 33× in this paper · explained in 2 episodes
• Metallicity — 27× in this paper · explained in 3 episodes
• Gravitational Wave Emission — 4× in this paper · explained in 2 episodes
• Abundance — 2× in this paper · explained in 1 episode
• Cluster Monte Carlo — 2× in this paper
• Laser Interferometer Space Antenna — 2× in this paper
• Population Synthesis — 2× in this paper · explained in 2 episodes
• Carnegie Astrophysics Summer Student Internship — 1× in this paper
• Mass Segregation — 1× in this paper · explained in 2 episodes
• Spectral Signature — 1× in this paper · explained in 2 episodes

Sources

• Machine Learning Methods for Stellar Collisions. I. Predicting Outcomes of SPH Simulations
• An analytical approach to binary populations in globular clusters
• GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
• Globular Cluster X-ray Sources
• Mass Distribution of Binary Black Hole Mergers from Young and Old Dense Star Clusters

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