The Characterization of the Dust Content in the Ring Around Sz 91: Indications of Planetesimal Formation?
Date Issued
2021-12
Author(s) USM
DOI
10.3847/1538-4357/ac21d0
Abstract
One of the most important questions in the field of planet formation is how millimeter- and centimeter-sized dust particles overcome radial drift and fragmentation barriers to form kilometer-sized planetesimals. ALMA observations of protoplanetary disks,
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