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Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed withChandraACIS

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V. Biffi, S. Borgani, G. Murante, E. Rasia, S. Planelles, G. L. Granato, C. Ragone-Figueroa, A. M. Beck, M. Gaspari and K. Dolag
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P. Arévalo, E. Churazov, I. Zhuravleva, W. R. Forman and C. Jones
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R. Kannan, M. Vogelsberger, G. S. Stinson, et al.
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The efficiency of magnetic field amplification at shocks by turbulence

Suoqing Ji (季索清), S. Peng Oh, M. Ruszkowski and M. Markevitch
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An implicit scheme for solving the anisotropic diffusion of heat and cosmic rays in the RAMSES code

Yohan Dubois and Benoît Commerçon
Astronomy & Astrophysics 585 A138 (2016)
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Analytical model for non-thermal pressure in galaxy clusters – II. Comparison with cosmological hydrodynamics simulation

Xun Shi, Eiichiro Komatsu, Kaylea Nelson and Daisuke Nagai
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Shaping the X-ray spectrum of galaxy clusters with AGN feedback and turbulence

M. Gaspari
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ON THE CLUSTER PHYSICS OF SUNYAEV–ZEL’DOVICH AND X-RAY SURVEYS. IV. CHARACTERIZING DENSITY AND PRESSURE CLUMPING DUE TO INFALLING SUBSTRUCTURES

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The Astrophysical Journal 806 (1) 43 (2015)
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The role of the artificial conductivity in SPH simulations of galaxy clusters: effects on the ICM properties

V. Biffi and R. Valdarnini
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An efficient Fokker–Planck solver and its application to stochastic particle acceleration in galaxy clusters

J. Donnert and G. Brunetti
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M. Gaspari, F. Brighenti, P. Temi and S. Ettori
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The relation between gas density and velocity power spectra in galaxy clusters: High-resolution hydrodynamic simulations and the role of conduction

M. Gaspari, E. Churazov, D. Nagai, E. T. Lau and I. Zhuravleva
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Filaments in the southern giant lobe of Centaurus A: constraints on nature and origin from modelling and GMRT observations

Sarka Wykes, Huib T. Intema, Martin J. Hardcastle, et al.
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Analytical model for non-thermal pressure in galaxy clusters

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Feedback, scatter and structure in the core of the PKS 0745-191 galaxy cluster

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