Compression of Dust Aggregates via Sequential Collisions with High Mass Ratios

The structure of dust aggregates affects many aspects of planet formation, such as the dust collision outcome, opacity, and radiation field. The millimeter-wave scattering polarization in protoplanerary disks indicates that dust aggregates have relatively compact structures with a volume-filling fac...

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Bibliographic Details
Main Authors: Hidekazu Tanaka, Ryoichi Anayama, Ryo Tazaki
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acb92b