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Accretion Does Not Drive the Turbulence in Galactic Disks

, , and . (2013)cite arxiv:1301.4500Comment: 7 pages, 3 figures, submitted to MNRAS.

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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)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.MUFASA: Galaxy star formation, gas, and metal properties across cosmic time, , , and . (2016)cite arxiv:1610.01626Comment: 19 pages, MNRAS submitted.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.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.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.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.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!.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.