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astro-ph.GA2024
Grain Size in the Class I Protostellar System TMC-1A Constrained with ALMA and VLA Observations
Yusuke Aso, Satoshi Ohashi, Hauyu Baobab Liu +1
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…
astro-ph.EP2024
SMA 200-400 GHz Survey for Dust Properties in the Icy Class II Disks in the Taurus Molecular Cloud
Chia-Ying Chung, Sean M. Andrews, Mark A. Gurwell +4
We present a new SMA survey of 47 Class II sources in the Taurus-Auriga region. Our observations made 12 independent samples of flux densities over the 200-400 GHz frequency range.…