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2017MNRAS.470.2018S - Mon. Not. R. Astron. Soc., 470, 2018-2033 (2017/September-2)
How does an asymmetric magnetic field change the vertical structure of a hot accretion flow?
SAMADI M., ABBASSI S. and LOVELACE R.V.E.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): accretion, accretion discs - black hole physics - magnetic fields - MHD - methods: numerical - methods: numerical
Simbad objects: 8
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