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

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...

Full description

Bibliographic Details
Main Authors: Marius Lehmann, Min-Kai Lin
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Hydrodynamics
Astrophysical fluid dynamics
Planet formation
Planetesimals
Online Access:https://doi.org/10.3847/1538-4357/ad496c

Internet

https://doi.org/10.3847/1538-4357/ad496c

Similar Items