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Streaming Instabilities in Accreting Protoplanetary Disks: A Parameter Study

The streaming instability (SI) is currently the leading candidate for triggering planetesimal formation in protoplanetary disks. Recently, a novel variation, the “azimuthal-drift” streaming instability (AdSI), was discovered in disks exhibiting laminar gas accretion. Unlike the classical SI, the AdS...

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Principais autores: Shiang-Chih Wang, Min-Kai Lin
פורמט: Artigo
שפה:Inglês
יצא לאור: IOP Publishing 2024-01-01
סדרה:The Astrophysical Journal
נושאים:
Planet formation
Protoplanetary disks
Magnetohydrodynamics
Astrophysical fluid dynamics
Hydrodynamical simulations
גישה מקוונת:https://doi.org/10.3847/1538-4357/ad862d
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