Dust Scattering Albedo at Millimeter Wavelengths in the TW Hya Disk

Dust Scattering Albedo at Millimeter Wavelengths in the TW Hya Disk

Planetary bodies are formed by coagulation of solid dust grains in protoplanetary disks. Therefore, it is crucial to constrain the physical and chemical properties of the dust grains. In this study, we measure the dust albedo at millimeter wavelength, which depends on dust properties at the disk mid...

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Bibliographic Details
Main Authors: Tomohiro C. Yoshida, Hideko Nomura, Takashi Tsukagoshi, Kiyoaki Doi, Kenji Furuya, Akimasa Kataoka
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Protoplanetary disks
Planet formation
Dust composition
Online Access:https://doi.org/10.3847/1538-4357/ad9f31
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