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Studying Binary Formation under Dynamical Friction Using Hill’s Problem

Using the equations of motion from Hill’s problem, with added accelerations for different forms of dynamical friction, we provide the (to-date) broadest scale-free study of friction-driven binary formation in gaseous disks and stellar clusters. We focus mainly on binary formation between stellar-mas...

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Bibliografische gegevens
Hoofdauteurs: Mark Dodici, Scott Tremaine
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal
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Online toegang:https://doi.org/10.3847/1538-4357/ad5cf2
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