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Cited article:

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Turbulent motions and shocks waves in galaxy clusters simulated with adaptive mesh refinement

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Astronomy & Astrophysics 504 (1) 33 (2009)
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ON THE ORIGIN OF COOL CORE GALAXY CLUSTERS: COMPARING X-RAY OBSERVATIONS WITH NUMERICAL SIMULATIONS

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Optical depth of the Universe to ultrahigh energy cosmic ray scattering in the magnetized large scale structure

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Physical Review D 77 (12) (2008)
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Cluster Merger Shock Constraints on Particle Acceleration and Nonthermal Pressure in the Intracluster Medium

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The Astrophysical Journal 675 (1) 126 (2008)
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Diffuse radio emission from clusters in the MareNostrum Universe simulation

M. Hoeft, M. Brüggen, G. Yepes, S. Gottlöber and A. Schwope
Monthly Notices of the Royal Astronomical Society 391 (4) 1511 (2008)
https://doi.org/10.1111/j.1365-2966.2008.13955.x

N‐Body + Magnetohydrodynamical Simulations of Merging Clusters of Galaxies: Characteristic Magnetic Field Structures Generated by Bulk Flow Motion

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The Astrophysical Journal 687 (2) 951 (2008)
https://doi.org/10.1086/592059

Structures of the magnetoionic media around the Fanaroff-Riley Class I radio galaxies 3C 31 and Hydra A

R. A. Laing, A. H. Bridle, P. Parma and M. Murgia
Monthly Notices of the Royal Astronomical Society 391 (2) 521 (2008)
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Magnetic fields and cosmic rays in galaxy clusters and large scale structures

Klaus Dolag, F. Stasyszyn, J. Donnert and R. Pakmor
Proceedings of the International Astronomical Union 4 (S259) 519 (2008)
https://doi.org/10.1017/S1743921309031202