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 …

We present the design and methods of the COS-Halos survey, a systematic investigation of
the gaseous halos of 44 z= 0.15–0.35 galaxies using background QSOs observed with the …

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 …

ABSTRACT We introduce Project GIBLE (Gas Is Better resoLved around galaxiEs), a suite of
cosmological zoom-in simulations where gas in the circumgalactic medium (CGM) is …

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 …

ABSTRACT The Milky Way's million degree gaseous halo contains a considerable amount
of mass that, depending on its structural properties, can be a significant mass component. In …

Recent observations have constrained the orbit and structure of the Large Magellanic Cloud
(LMC), implying a well-constrained pericentric passage about the Milky Way (MW)∼ 50 Myr …

We examine how Hi and metal absorption lines within low-redshift galaxy haloes trace the
dynamical state of circumgalactic gas, using cosmological hydrodynamic simulations that …

Dynamic interactions between the two Magellanic Clouds have flung large quantities of gas
into the halo of the Milky Way. The result is a spectacular arrangement of gaseous …