Constraints on the Dust Size Distributions in the HD 163296 Disk from the Difference of the Apparent Dust Ring Widths between Two ALMA Bands

Constraints on the Dust Size Distributions in the HD 163296 Disk from the Difference of the Apparent Dust Ring Widths between Two ALMA Bands

The dust size in protoplanetary disks is a crucial parameter for understanding planet formation, while the observational constraints on dust size distribution have large uncertainties. In this study, we present a new method to constrain the dust size distribution from the dust spatial distribution,...

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Bibliographic Details
Main Authors: Kiyoaki Doi, Akimasa Kataoka
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Planet formation
Submillimeter astronomy
Dust continuum emission
Dust physics
Online Access:https://doi.org/10.3847/1538-4357/acf5df

Internet

https://doi.org/10.3847/1538-4357/acf5df

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