Three-dimensional Global Simulations of Type-II Planet–Disk Interaction with a Magnetized Disk Wind. I. Magnetic Flux Concentration and Gap Properties

Three-dimensional Global Simulations of Type-II Planet–Disk Interaction with a Magnetized Disk Wind. I. Magnetic Flux Concentration and Gap Properties

Giant planets embedded in protoplanetary disks (PPDs) can create annulus density gaps around their orbits in the type-II regime, potentially responsible for the ubiquity of annular substructures observed in PPDs. Although a substantial amount of works studying type-II planetary migration and gap pro...

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Bibliographic Details
Main Authors: Yuhiko Aoyama, Xue-Ning Bai
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Magnetohydrodynamical simulations
Protoplanetary disks
Planet formation
Planetary migration
Planetary-disk interactions
Hydrodynamical simulations
Online Access:https://doi.org/10.3847/1538-4357/acb81f

Internet

https://doi.org/10.3847/1538-4357/acb81f

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