A Three-dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk Using DCO

Gas kinematics are an important part of the planet formation process. Turbulence influences planetesimal growth and migration from the scale of submicron dust grains through gas-giant planets. Radio observations of resolved molecular line emission can directly measure this non-thermal motion and, ta...

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Bibliographic Details

Published in:	The Astrophysical journal 2017-07, Vol.843 (2), p.150
Main Authors:	Flaherty, Kevin M., Hughes, A. Meredith, Rose, Sanaea C., Simon, Jacob B., Qi, Chunhua, Andrews, Sean M., Kóspál, Ágnes, Wilner, David J., Chiang, Eugene, Armitage, Philip J., Bai, Xue-ning
Format:	Article
Language:	eng
Subjects:	ACCRETION DISKS accretion, accretion disks Astrochemistry Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CARBON 18 CARBON MONOXIDE COMPUTERIZED SIMULATION COSMIC DUST COSMIC GASES DEUTERIUM COMPOUNDS EMISSION Emission measurements FORECASTING Gas giant planets INSTABILITY Kinematics Magnetic fields Molecular structure MOLECULES Organic chemistry Planet formation PLANETS Protoplanetary disks PROTOPLANETS Radio observation STARS stars: individual (HD 163296) THREE-DIMENSIONAL CALCULATIONS TURBULENCE
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