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FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation

, , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1702.06148Comment: 66 pages, 39 figures. Simulation animations and visualizations available at http://www.tapir.caltech.edu/~phopkins/Site/animations and http://fire.northwestern.edu Paper includes complete FIRE algorithms and public ICs (http://www.tapir.caltech.edu/~phopkins/publicICs).

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Modeling chemical abundance distributions for dwarf galaxies in the Local Group: the impact of turbulent metal diffusion, , , , , , , , and . (Oct 18, 2017)Gusty, gaseous flows of FIRE: galactic winds in cosmological simulations with explicit stellar feedback, , , , , and . (2015)cite arxiv:1501.03155Comment: 23 pages, 12 figures, submitted to MNRAS; comments welcome.MUFASA: Galaxy star formation, gas, and metal properties across cosmic time, , , and . (2016)cite arxiv:1610.01626Comment: 19 pages, MNRAS submitted.When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies, , , , , , , and . (2016)cite arxiv:1610.04232Comment: Submitted to ApJ. Main results in Figures 3, 7, and 8.An instability of feedback regulated star formation in galactic nuclei, , , , , , and . (2016)cite arxiv:1601.07186Comment: 14 pages; 11 figures; submitted to MNRAS; comments welcome. Animations of the isolated disks presented in this paper can be found at http://www.mit.edu/~ptorrey/media.html#iso_disks.How To Model Supernovae in Simulations of Star and Galaxy Formation, , , , , , , , and . (2017)cite arxiv:1707.07010Comment: 16 pages, 9 figures (+8 pages, 5 figures in appendices). Submitted to MNRAS.Physical models of streaming instabilities in protoplanetary disks, and . (2020)cite arxiv:2003.01738.The first light from tidal disruption events, , and . (2020)cite arxiv:2012.12271Comment: 22 pages, 19 figures, submitted to MNRAS. Movies of the simulation are available at http://www.tapir.caltech.edu/~bonnerot/first-light.html. Comments welcome!.No missing photons for reionization: moderate ionizing photon escape fractions from the FIRE-2 simulations, , , , , and . (2020)cite arxiv:2003.05945Comment: 16 pages, 11 figures, submitted to MNRAS, comments welcome. Core results are shown in Fig 5 and Fig 7.An instability of feedback regulated star formation in galactic nuclei, , , , , , and . (Jan 26, 2016)