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20242026
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astro-ph.GA2026

The Prevalence of Turbulence-Regulated Multiphase Galactic Winds in Star-Forming Galaxies

Zhihui Li, Timothy Heckman, Max Gronke +8

We build upon our previously developed multi-ion radiative transfer (RT) framework, PEACOCK, to investigate the kinematic and energetic structure of cool-to-warm galactic winds in…

astro-ph.GA2026

Kinematically Coherent Multiphase Galactic Winds in Star-Forming Galaxies Revealed by Unified Radiative Transfer Modeling of UV Emission and Absorption Lines

Zhihui Li, Timothy Heckman, Max Gronke +8

We present PEACOCK, a three-dimensional Monte Carlo radiative transfer (RT) framework designed to self-consistently model rest-frame ultraviolet emission and absorption lines arisi…

astro-ph.GA2026

Effects of Numerical Resolution on Simulated Cloud-Wind Interactions

Hannah Leary, Helena M. Richie, Evan Schneider

Mixing by hydrodynamical instabilities plays a key role in cloud-wind interactions, causing cloud destruction in the adiabatic limit and facilitating cloud survival with efficient…

astro-ph.GA2026

Simulations of multi-phase gas in and around galaxies

Max Gronke, Evan Schneider

Multiphase gas -- ranging from cold molecular clouds (K) to hot, diffuse plasma (K) is a defining feature of the interstellar, circumgalactic, intra…

astro-ph.GA2025

Dust Evolution in Simulated Multiphase Galactic Outflows

Helena M. Richie, Evan E. Schneider

We present the first large-scale, high-resolution simulations of dusty, star formation feedback-driven galactic outflows. Using the Cholla hydrodynamics code, we investigate dust s…

astro-ph.GA2025

Resolution Dependence of Cloud-Wind Simulations

Hannah J. Leary, Evan Schneider, Helena M. Richie

Using a set of wind-tunnel simulations, we investigate the effect that numerical resolution has on cloud evolution and acceleration. We also consider the role of wind speed in both…