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Dynamical Processes in the Planet-Forming Environment

Published onMay 31, 2019
Dynamical Processes in the Planet-Forming Environment
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Abstract

The transfer of circumstellar disk mass and momentum onto the protostar and out into the environment occurs via a variety of mechanisms including magnetospheric accretion, jets, outflows, and disk winds. Metallic emission lines, along with the Balmer series of hydrogen, probe the kinematics of gas within the planet-forming regions of the disks.

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