We present a novel analytic framework to model the steady-state structure of multiphase
galactic winds comprised of a hot, volume-filling component and a cold, clumpy component …

We analyse the physical properties of gas in the circumgalactic medium (CGM) of 132 Milky
Way (MW)-like galaxies at z= 0 from the cosmological magneto-hydrodynamical simulation …

We characterize mass, momentum, energy, and metal outflow rates of multiphase galactic
winds in a suite of FIRE-2 cosmological 'zoom-in'simulations from the Feedback in Realistic …

We present cosmological hydrodynamic simulations of a quasar-mass halo (M halo≈ 10
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …

Abstract The hot (> 10 6 K) phase of the circumgalactic medium (CGM) contains a large
fraction of baryons in galaxies. It also retains signatures of the processes that shaped the …

We present a study of the metal-enriched halo gas, traced using Mg ii and [O ii] emission
lines, in two large, blind galaxy surveys–the MUSE (Multi Unit Spectroscopic Explorer) …

Using high-resolution Romulus simulations, we explore the origin and evolution of the
circumgalactic medium (CGM) in the region 0.1≤ R/R 500≤ 1 around massive central …

We revisit the problem of the growth of dense/cold gas in the cloud-crushing set-up with
radiative cooling. The relative motion between the dense cloud and the diffuse medium …

Using the state-of-the-art suite of hydrodynamic simulations Simba, as well as its dark-matter-
only counterpart, we study the impact of the presence of baryons and of different stellar/AGN …

We present a novel set of stellar feedback models, implemented in the moving-mesh code
arepo, designed for galaxy formation simulations with near-parsec (or better) resolution …