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Young Star Clusters Dominate the Production of Detached Black Hole–Star Binaries

The recent discovery of two detached black hole–star (BH–star) binaries from Gaia’s third data release has sparked interest in understanding the formation mechanisms of these systems. We investigate the formation of these systems by dynamical processes in young star clusters (SCs) and via isolated b...

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Hlavní autoři: Ugo Niccolò Di Carlo, Poojan Agrawal, Carl L. Rodriguez, Katelyn Breivik
Médium: Artigo
Jazyk:Inglês
Vydáno: IOP Publishing 2024-01-01
Edice:The Astrophysical Journal
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On-line přístup:https://doi.org/10.3847/1538-4357/ad2f2c
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