Grain Size in the Class I Protostellar System TMC-1A Constrained with ALMA and Very Large Array Observations

Grain Size in the Class I Protostellar System TMC-1A Constrained with ALMA and Very Large Array Observations

The disk mass and substructure in young stellar objects suggest that planet formation may start at the protostellar stage, through the growth of dust grains. To accurately estimate the grain size at the protostellar stage, we have observed the Class I protostar TMC-1A using the Jansky Very Large Arr...

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Bibliographic Details
Main Authors: Yusuke Aso, Satoshi Ohashi, Hauyu Baobab Liu, Wenrui Xu
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Circumstellar disks
Circumstellar grains
Protostars
Low mass stars
Online Access:https://doi.org/10.3847/1538-4357/ad938e

Internet

https://doi.org/10.3847/1538-4357/ad938e

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