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A Long Period Stellar-mass Black Hole Binary in ω Centauri

Modern simulations of stellar dynamics in globular clusters peg a dominant role for stellar-mass black holes, but direct evidence for black holes in clusters remains limited. We present the discovery of an astrometric stellar-mass black hole–main sequence star binary in ω Centauri, the most massive...

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Principais autores: Matthew Whitaker, Evan Kerr, Anil Seth, Maximilian Häberle, Jay Strader, Jay Anderson, Andrea Bellini, Callie Clontz, Zack Freeman, Massimo Griggio, Sebastian Kamann, Mattia Libralato, Nadine Neumayer, Elena González Prieto, Carl L. Rodriguez, Sara Saracino, Peter Smith, Glenn van de Ven, Zixian Wang
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2026-01-01
Serier:The Astrophysical Journal Letters
Fag:
Stellar mass black holes
Black holes
Globular star clusters
Astrometric binary stars
Binary stars
Astrometry
Online adgang:https://doi.org/10.3847/2041-8213/ae7a5c
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