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2022ApJ...930..111D - Astrophys. J., 930, 111-111 (2022/May-2)
Clumpy Accretion in Pre-main-sequence Stars as a Source of Perturbations in Circumstellar Disks.
DEMIDOVA T.V. and GRININ V.P.
Abstract (from CDS):
Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.
Journal keyword(s): Accretion - Protoplanetary disks - Pre-main sequence stars - Hydrodynamical simulations - Radiative transfer simulations
Simbad objects: 14
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