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The Hydrangea simulations: galaxy formation in and around massive clusters

, , , , , , , , , , , , , , and . (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.

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The environmental dependence of gas accretion onto galaxies: quenching satellites through starvation, , , , , , and . (2016)cite arxiv:1611.03870Comment: Submitted to MNRAS. Comments welcome.EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies, , , , , , , and . (2022)cite arxiv:2210.09978.The environmental dependence of HI in galaxies in the EAGLE simulations, , , , , , and . (2016)cite arxiv:1606.06288Comment: 23 pages, 16 figures, accepted for publication by MNRAS.The Hydrangea simulations: galaxy formation in and around massive clusters, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1703.10907Comment: 20 pages, 15 figures, submitted to MNRAS.The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1511.04909Comment: 23 pages, 17 figures (16 pages, 9 figures without appendices), accepted by MNRAS.The origin of the enhanced metallicity of satellite galaxies, , , , , , , and . (2016)cite arxiv:1609.03379Comment: 22 pages, 15 figures; accepted by MNRAS.