Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region
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Abstract
Rings are the most frequently revealed substructure in ALMA dust observations of protoplanetary disks, but their origin is still hotly debated. In this paper, we identify dust substructures in 12 disks and measure their properties to investigate how they form. This subsample of disks is selected from a high-resolution (
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1538-4357