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Three-Dimensional MHD Simulations of a Subcluster Plasma Moving in Turbulent ICM
Published online by Cambridge University Press: 01 August 2006
Abstract
We carried out 3D magnetohydrodynamic simulations of a subcluster moving in turbulent ICM by including anisotropic heat conduction. Since magnetic fields stretched along the subcluster surface suppress the heat conduction across the front, cold fronts are formed and sustained.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 189
- Copyright
- Copyright © International Astronomical Union 2007