Evolution and structure of magnetic fields in simulated galaxy clusters
We use cosmological magneto-hydrodynamic simulations to study the evolution of magnetic fields in galaxy clusters in two different cosmological models, a standard-CDM and a $\Lambda$-CDM model. We show that the magnetic field strength profiles closely follow the cluster density profiles outside a co...
Saved in:
| Main Authors: | , , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
February 1, 2008
|
| In: |
Arxiv
|
| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/0202272
|
| Author Notes: | Klaus Dolag, Matthias Bartelmann, and Harald Lesch |
Search Result 1
Evolution and structure of magnetic fields in simulated galaxy clusters
Article (Journal)
Online Resource