On Secular Gravitational Instability in Vertically Stratified Disks

On Secular Gravitational Instability in Vertically Stratified Disks

Secular gravitational instability (GI) is one promising mechanism for explaining planetesimal formation. Previous studies of secular GI utilized a razor-thin disk model and derived the growth condition in terms of vertically integrated physical values such as dust-to-gas surface density ratio. Howev...

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Bibliographic Details
Main Authors: Ryosuke T. Tominaga, Shu-ichiro Inutsuka, Sanemichi Z. Takahashi
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Hydrodynamics
Astrophysical fluid dynamics
Online Access:https://doi.org/10.3847/1538-4357/ace043

Internet

https://doi.org/10.3847/1538-4357/ace043

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