Introduction

High-redshift analogue Evolution of 1, 0.1, 0.01, and 0.001 micron radius dust grains (from left to right) under sputtering in a multi-phase galactic outflow. The galaxy has a star formation rat...

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...