Convective Overstability in Radially Global Protoplanetary Disks. I. Pure Gas Dynamics

Protoplanetary disks are prone to several hydrodynamic instabilities. One candidate, convective overstability (COS), can drive radial semiconvection that may influence dust dynamics and planetesimal formation. However, the COS has primarily been studied in local models. This paper investigates the C...

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Detalhes bibliográficos

Principais autores:	Marius Lehmann, Min-Kai Lin
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2024-01-01
coleção:	The Astrophysical Journal
Assuntos:	Protoplanetary disks Hydrodynamics Astrophysical fluid dynamics Planet formation Planetesimals
Acesso em linha:	https://doi.org/10.3847/1538-4357/ad496c
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