The Roles of Dust Growth in the Temperature Evolution and Snow Line Migration in Magnetically Accreting Protoplanetary Disks

The Roles of Dust Growth in the Temperature Evolution and Snow Line Migration in Magnetically Accreting Protoplanetary Disks

The temperature structure of protoplanetary disks provides an important constraint on where in the disks rocky planets like our own form. Recent nonideal magnetohydrodynamical (MHD) simulations have shown that the internal Joule heating associated with magnetically driven disk accretion is inefficie...

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Bibliographic Details
Main Authors: Katsushi Kondo, Satoshi Okuzumi, Shoji Mori
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Magnetohydrodynamics
Planet+ formation
Solar system terrestrial planets
Online Access:https://doi.org/10.3847/1538-4357/acc840

Internet

https://doi.org/10.3847/1538-4357/acc840

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