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

Published in:	The Astrophysical Journal
Main Authors:	Ryota Yamamuro, Kei E. I. Tanaka, Satoshi Okuzumi
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Subjects:	Protoplanetary disks Protostars Massive stars Stellar accretion disks Star formation Planetesimals
Online Access:	https://doi.org/10.3847/1538-4357/adf49c