The gas surrounding galaxies outside their disks or interstellar medium and inside their virial
radii is known as the circumgalactic medium (CGM). In recent years this component of …

Galactic halo gas traces inflowing star-formation fuel and feedback from a galaxy's disk and
is therefore crucial to our understanding of galaxy evolution. In this review, we summarize …

We present simulations from the new" Figuring Out Gas & Galaxies in Enzo"(FOGGIE)
project. In contrast to most extant simulations of galaxy formation, which concentrate …

Abstract The precise localization (< 1 arcsec) of multiple fast radio bursts (FRBs) to> 0.1
galaxies has confirmed that the dispersion measures (DMs) of these enigmatic sources …

The circumgalactic medium (CGM) is fed by galaxy outflows and accretion of intergalactic
gas, but its mass, heavy element enrichment, and relation to galaxy properties are poorly …

We present a budget and accounting of metals in and around star-forming galaxies at z∼ 0.
We combine empirically derived star formation histories with updated supernova and …

The circumgalactic medium (CGM) of late-type galaxies is characterized using UV
spectroscopy of 11 targeted QSO/galaxy pairs at z⩽ 0.02 with the Hubble Space Telescope …

We use the TNG50 simulation of the IllustrisTNG project to study cold, dense clouds of gas in
the circumgalactic media (CGM) of Milky Way-like galaxies. We find that their CGM is …

The Magellanic Clouds are surrounded by an extended network of gaseous structures. Chief
among these is the Magellanic Stream, an interwoven tail of filaments trailing the Clouds in …

Numerical simulations predict that metal-poor gas accretion from the cosmic web fuels the
formation of disk galaxies. This paper discusses how cosmic gas accretion controls star …