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 …

We present an analysis of the galaxy-scale gaseous outflows from the Feedback in Realistic
Environments (FIRE) simulations. This suite of hydrodynamic cosmological zoom …

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 analyze new far-ultraviolet spectra of 13 quasars from the~ z 0.2 COS-Halos survey
that cover the Hi Lyman limit of 14 circumgalactic medium (CGM) systems. These data …

We use a particle tracking analysis to study the origins of the circumgalactic medium (CGM),
separating it into (1) accretion from the intergalactic medium (IGM),(2) wind from the central …

Context. The existence of magnetic fields in the circumgalactic medium (CGM) is largely
unconstrained. Their detection is important as magnetic fields can have a significant impact …

The TNG50 cosmological simulation produces X-ray emitting bubbles, shells, and cavities in
the circumgalactic gas above and below the stellar discs of Milky Way-and Andromeda-like …

We summarize and reanalyze observations bearing on missing galactic baryons, where we
propose a consistent picture for halo gas in L≳ L* galaxies. The hot X-ray-emitting halos are …

We construct an analytic phenomenological model for extended warm/hot gaseous coronae
of L* galaxies. We consider UV O vi Cosmic Origins Spectrograph (COS)-Halos absorption …

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 …