2D Magnetohydrodynamics simulations of induced plasma dynamics in the near-core region of a galaxy cluster
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/410/4/2602/6296038/mnras0410-2602.pdf
Reference121 articles.
1. The Origin of Cold Fronts in the Cores of Relaxed Galaxy Clusters
2. Stability, Instability, and “Backward” Transport in Stratified Fluids
3. Regulation of Thermal Conductivity in Hot Galaxy Clusters by MHD Turbulence
4. Total Variation Diminishing Scheme for Adiabatic and Isothermal Magnetohydrodynamics
5. The role of heat conduction in the cooling flows of galaxy clusters
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