Magneto-thermal instability in galaxy clusters - I. Theory and two-dimensional simulations (2022)
Attributed to:
Magnetic dynamos and magnetic flux evolution in accretion disk turbulence
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stac974
Publication URI: http://dx.doi.org/10.1093/mnras/stac974
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3