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2017MNRAS.470.2938F - Mon. Not. R. Astron. Soc., 470, 2938-2948 (2017/September-3)
Reorienting MHD colliding flows: a shock physics mechanism for generating filaments normal to magnetic fields.
FOGERTY E., CARROLL-NELLENBACK J., FRANK A., HEITSCH F. and PON A.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): MHD - stars: formation - ISM: clouds - ISM: kinematics and dynamics - ISM: structure - ISM: structure
Simbad objects: 5
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