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2020MNRAS.495.3795W - Mon. Not. R. Astron. Soc., 495, 3795-3806 (2020/July-2)
Non-ideal magnetohydrodynamics versus turbulence - I. Which is the dominant process in protostellar disc formation?
WURSTER J. and LEWIS B.T.
Abstract (from CDS):
Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): magnetic fields - MHD - turbulence - protoplanetary discs - stars: formation - stars: winds, outflows
Simbad objects: 1
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