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The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D, , , , , , и . (2014)cite arxiv:1412.6105Comment: 12 pages, 10 figures, submitted to MNRAS.Temperature Structure of the Intra-Cluster Medium from SPH and AMR simulations, , , , , , , , , и 1 other автор(ы). (17.06.2014)nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region, , , , , , , , , и 12 other автор(ы). (2016)cite arxiv:1609.07311Comment: 14 pages, 9 figures, 1 table; accepted for publication in MNRAS.Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping, , , , , , , , , и 1 other автор(ы). (2015)cite arxiv:1510.04277Comment: 18 pages, 12 figures. Comments welcome.A warm mode of gas accretion on forming galaxies, , , , , и . (2012)cite arxiv:1202.5212Comment: 6 pages, 3 figures, accepted for publication in ApJL.nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes, , , , , , , , , и 10 other автор(ы). (2015)cite arxiv:1511.08255Comment: 17 pages (+4 page appendix), 16 figures, 2 tables; submitted to MNRAS.nIFTy galaxy cluster simulations I: dark matter & non-radiative models, , , , , , , , , и 17 other автор(ы). (2015)cite arxiv:1503.06065Comment: 21 pages, 13 figures, 4 tables - submitted to MNRAS.Shall numerical astrophysics step into the era of Exascale computing?, , , , , , , и . CoRR, (2019)