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Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation

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Metal flows of the circumgalactic medium, and the metal budget in galactic halos, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1606.09252Comment: 18 Pages, 14 Figures, Submitted to MNRAS, comments welcome.The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations, , , , , and . (2016)cite arxiv:1610.08523Comment: 22 pages, 17 figures, Submitted to MNRAS.Massive blue early-type galaxies in the SDSS. I. A new population of recently quenched elliptical galaxies, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1308.0054Comment: 25 pages, 9 figures. Submitted to MNRAS. Version with full resolution figures at http://cas.umkc.edu/physics/mcintosh/mcintosh.RQE.hires.pdf.First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations, , , , , , and . (2021)cite arxiv:2109.09762Comment: 30 pages, 15 figures, submitted to MNRAS. Comments welcome.Giant clumps in the FIRE simulations: a case study of a massive high-redshift galaxy, , , , , and . (2016)cite arxiv:1603.03778Comment: 16 pages, 14 figures; submitted to MNRAS.Reconciling dwarf galaxies with LCDM cosmology: Simulating a realistic population of satellites around a Milky Way-mass galaxy, , , , , and . (2016)cite arxiv:1602.05957Comment: 6 pages, 5 figures. Submitted to ApJ Letters.Star(bursts) of FIRE: observational signatures of bursty star formation in galaxies, , , , , , and . (2015)cite arxiv:1510.03869Comment: 21 pages, 15 figures, submitted to MNRAS.FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation, , , , , , , , , and 18 other author(s). (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).Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation, , , , , , and . (Jul 18, 2016)The Difficulty Getting High Escape Fractions of Ionizing Photons from High-redshift Galaxies: a View from the FIRE Cosmological Simulations, , , , , , and . (2015)cite arxiv:1503.07880Comment: 16 pages, 14 figures, submitted to MNRAS; comments welcome.