SIGNATURES OF MRI-DRIVEN TURBULENCE IN PROTOPLANETARY DISKS: PREDICTIONS FOR ALMA OBSERVATIONS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/808/i=2/a=180/pdf
Reference86 articles.
1. Evolution of Molecular Abundance in Gaseous Disks around Young Stars: Depletion of CO Molecules
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