Gravitational Instability, Spiral Substructure, and Modest Grain Growth in a Typical Protostellar Disk: Modeling Multiwavelength Dust Continuum Observations of TMC1A

Gravitational Instability, Spiral Substructure, and Modest Grain Growth in a Typical Protostellar Disk: Modeling Multiwavelength Dust Continuum Observations of TMC1A

Embedded class 0/I protostellar disks represent the initial condition for planet formation. This calls for a better understanding of their bulk properties and the dust grains within them. We model multiwavelength dust continuum observations of the disk surrounding the class I protostar TMC1A to prov...

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Bibliographic Details
Main Authors: Wenrui Xu, Satoshi Ohashi, Yusuke Aso, Hauyu Baobab Liu
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Gravitational instability
Dust continuum emission
Astronomy data modeling
Planet formation
Online Access:https://doi.org/10.3847/1538-4357/aced4c

Internet

https://doi.org/10.3847/1538-4357/aced4c

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