Galactic winds shape the stellar, gas, and metal content of galaxies. To quantify their impact,
we must understand their physics. We review potential wind-driving mechanisms and …

Galaxy evolution is an important topic, and our physical understanding must be complete to
establish a correct picture. This includes a thorough treatment of feedback. The effects of …

Galaxies comprise intricate networks of interdependent processes which together govern
their evolution. Central among these are the multiplicity of feedback channels, which remain …

We model the stellar abundances and ages of two disrupted dwarf galaxies in the Milky Way
stellar halo: Gaia-Sausage Enceladus (GSE) and Wukong/LMS-1. Using a statistically robust …

Context. Lyman break analogs in the local Universe serve as counterparts to Lyman break
galaxies (LBGs) at high redshifts, which are widely regarded as major contributors to cosmic …

We construct simulated galaxy data sets based on the High Energy X-ray Probe (HEX-P)
mission concept to demonstrate the significant advances in galaxy science that will be …

The recent decade has seen an exponential growth in spatially resolved metallicity
measurements in the interstellar medium (ISM) of galaxies. To first order, these …

Context. Massive star formation leads to enrichment of the interstellar medium with heavy
elements. On the other hand, the abundance of heavy elements is a key parameter with …

We present the spatially resolved measurements of a cool galactic outflow in the
gravitationally lensed galaxy RCS0327 at z≈ 1.703 using VLT/MUSE IFU observations. We …

Stellar feedback-driven outflows are important regulators of the gas–star formation cycle.
However, resolving outflow physics requires high-resolution observations that can only be …