Introduction

This post is a summary of Richie et al. 2024, my first paper on dust evolution in galactic outflows. In this paper, we used idealized simulations of individual dusty clouds in hot galactic winds to...

When simulating dust, a major simplification in modeling can be made through assumptions about dust dynamics. Dust dynamics (which aren’t straightforward to calculate in Eulerian hydrodynamics simu...

Overview To understand how dust is transported in galactic winds, I’ve been thinking about the primary mechanism that destroys dust at high gas temperatures in galaxies, sputtering. In very simpl...