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Moving mesh cosmology: tracing cosmological gas accretion

, , , , , , and . (2013)cite arxiv:1301.6753Comment: 21 pages, 12 figures. MNRAS accepted (in press). High-resolution images can be found at http://www.cfa.harvard.edu/itc/research/movingmeshcosmology/.
DOI: 10.1093/mnras/sts595

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Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations, , , and . (2017)cite arxiv:1703.05766Comment: 23 pages, 11 figures, 3 tables, submitted to MNRAS.Moving mesh cosmology: numerical techniques and global statistics, , , , and . (2011)cite arxiv:1109.1281 Comment: 30 pages, 25 figures, submitted to MNRAS. Volume-rendering movies and high-resolution images can be found http://www.cfa.harvard.edu/itc/research/movingmeshcosmology.Resolving flows around black holes: the impact of gas angular momentum, and . (Jun 8, 2016)Moving mesh cosmology: the hydrodynamics of galaxy formation, , , , and . (2011)cite arxiv:1109.3468Comment: 29 pages, 27 figures, MNRAS submitted. Movies and high-resolution images can be found at http://www.cfa.harvard.edu/itc/research/movingmeshcosmology/.Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics, , and . (2017)cite arxiv:1709.03515Comment: 33 pages, 24 figures, submitted to MNRAS.The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite, , , , , , and . (2017)cite arxiv:1706.04790Comment: 16 pages, 8 figures, submitted to MNRAS.Morphological evolution of supermassive black hole merger hosts and multimessenger signatures, , , , , and . (2020)cite arxiv:2012.00775Comment: 14 pages, 17 figures. Submitted to MNRAS.Interpreting ALMA Observations of the ISM During the Epoch of Reionisation, , , and . (2016)cite arxiv:1612.01786Comment: 32 Pages, 25 figures, Submitted to MNRAS, Abstract abridged for arXiv.The impact of feedback on cosmological gas accretion, , , , , , and . (2014)cite arxiv:1410.5425Comment: 16 pages, 12 figures. MNRAS submitted, comments welcome. The official Illustris website can be found at http://www.illustris-project.org.The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1411.0667Comment: 11 pages, 9 figures. Submitted to MNRAS, comments welcome. The official Illustris website can be found at http://www.illustris-project.org/.