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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)

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Auroral radio emission from late L and T dwarfs: A new constraint on dynamo theory in the substellar regime, , , , , , and . (Nov 11, 2015)Modeling chemical abundance distributions for dwarf galaxies in the Local Group: the impact of turbulent metal diffusion, , , , , , , , and . (Oct 18, 2017)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).