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  1. Ceci n'est pas une Couche de Mélange: The Meaning of Resolved Turbulent Radiative Mixing

    Publication
    Turbulent Radiative Mixing Layers (TRMLs) are of fundamental importance to the transport of energy and momentum in multi-phase, astrophysical fluids. We use measurements of the "micro" and …

  2. Blue Monsters and Dusty Descendants: Reconciling UV and IR Emission from Galaxies from z \(\sim\) 7, up to z = 14

    Publication
    Recent JWST observations reveal massive, UV-bright galaxies at z>10 with little apparent dust attenuation, whereas ALMA detections at z≃7 show similarly massive systems that are …

  3. Taming the Tarantula: How Stellar Wind Feedback Shapes Gas and Dust in 30 Doradus

    Publication
    Observations of massive star-forming regions show that classical stellar wind models over-predict the luminosity of the X-ray emitting gas, indicating a significant fraction of wind …

  4. Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z > 10

    Publication
    The number density of UV luminous galaxies discovered by the James Webb Space Telescope at ultra high redshift (z ≳ 10) is higher, and declines much more slowly with …

  5. Suppression of Shock X-Ray Emission in Novae from Turbulent Mixing with Cool Gas

    Publication
    Shock interaction in classical novae occurs when a fast outflow from the white dwarf $\gtrsim\(1000 km s\)^{‑1}$ collides with a slower, cooler shell of …

  6. The Coevolution of Stellar Wind-blown Bubbles and Photoionized Gas. II. 3D RMHD Simulations and Tests of Semianalytic Models

    Publication
    In a companion paper (Paper I), we presented a coevolution model (CEM) in which to consider the evolution of feedback bubbles driven by massive stars through both stellar …

  7. The Coevolution of Stellar Wind-blown Bubbles and Photoionized Gas. I. Physical Principles and a Semianalytic Model

    Publication
    We propose a new framework for the simultaneous feedback of stellar winds and photo-ionizing radiation from massive stars, distinguishing the locations where forces are applied, and consequences …

  8. The Interplay between the Initial Mass Function and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities

    Publication
    The observed rest-UV luminosity function at cosmic dawn (\(z \sim 8-14\)) measured by JWST revealed an excess of UV-luminous galaxies relative to many pre-launch …