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  1. A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics

    Publication
    The circumgalactic medium (CGM) plays a pivotal role in regulating gas flows around galaxies and thus shapes their evolution. However, the details of how galaxies and their CGM …

  2. Code Comparison in Galaxy-scale Simulations with Resolved Supernova Feedback: Lagrangian versus Eulerian Methods

    Publication
    We present a suite of high-resolution simulations of an isolated dwarf galaxy using four different hydrodynamical codes: {sc Gizmo}, {sc Arepo}, {sc Gadget}, and {sc Ramses}. All …

  3. A Bayesian Population Model for the Observed Dust Attenuation in Galaxies

    Publication
    Dust plays a pivotal role in determining the observed spectral energy distribution (SED) of galaxies. Yet our understanding of dust attenuation is limited and our observations suffer from …

  4. Characterizing mass, momentum, energy, and metal outflow rates of multiphase galactic winds in the FIRE-2 cosmological simulations

    Publication
    We characterize mass, momentum, energy and metal outflow rates of multi-phase galactic winds in a suite of FIRE-2 cosmological "zoom-in" simulations from the Feedback in …

  5. A Solar System formation analogue in the Ophiuchus star-forming complex

    Publication
    Anomalies among the daughter nuclei of the extinct short-lived radionuclides (SLRs) in the calcium-aluminum-rich inclusions (CAIs) indicate that the Solar System must have been born …

  6. A Framework for Multiphase Galactic Wind Launching Using TIGRESS

    Publication
    Galactic outflows have density, temperature, and velocity variations at least as large as that of the multiphase, turbulent interstellar medium (ISM) from which they originate. We have conducted …

  7. A PDF PSA, or Never gonna set_xscale again -- guilty feats with logarithms

    Publication
    In the course of doing astronomy, one often encounters plots of densities, for example probability densities, flux densities, and mass functions. Quite frequently the ordinate of these diagrams …