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Dust growth and dust trapping in protoplanetary disks with the ngVLA

Published onMay 31, 2019
Dust growth and dust trapping in protoplanetary disks with the ngVLA
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Abstract

ALMA reveals structures in protoplanetary disks that indicate dust trapping as an important mechanism in the planet formation process, but interpretation is limited due to the optically thick mm emission. The next-generation Very Large Array (ngVLA) will open up the possibilities to study dust growth in disks in optically thin cm wavelengths.

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