The Impact of Silicate Grain Coagulation on Millimeter Emission from Massive Protostellar Disks

Hot accretion disks around massive protostars provide a unique opportunity to study ice-free silicate grains that cannot be investigated in protoplanetary disks. We conduct a self-consistent investigation into grain-size evolution and its impact on (sub)millimeter-wave emission from massive protoste...

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Bibliographic Details
Main Authors: Ryota Yamamuro, Kei E. I. Tanaka, Satoshi Okuzumi
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adf49c
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