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2016ApJ...821....3M - Astrophys. J., 821, 3-3 (2016/April-2)
Dust dynamics in protoplanetary disk winds driven by magnetorotational turbulence: a mechanism for floating dust grains with characteristic sizes.
MIYAKE T., SUZUKI T.K. and INUTSUKA S.-I.
Abstract (from CDS):
Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.
Journal keyword(s): accretion, accretion disks - dust, extinction - ISM: jets and outflows - planets and satellites: formation - protoplanetary disks - stars: pre-main sequence
Simbad objects: 1
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