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2020MNRAS.492.5641T - Mon. Not. R. Astron. Soc., 492, 5641-5654 (2020/March-2)
Star-disc alignment in the protoplanetary discs: SPH simulation of the collapse of turbulent molecular cloud cores.
TAKAISHI D., TSUKAMOTO Y. and SUTO Y.
Abstract (from CDS):
Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): hydrodynamics - turbulence - methods: numerical - protoplanetary discs - stars: protostars
Simbad objects: 9
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