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 …

ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …

We present a series of high-resolution cosmological simulations1 of galaxy formation to z=
0, spanning halo masses∼ 108–1013 M⊙, and stellar masses∼ 104–1011 M⊙. Our …

This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …

We analyze the physical conditions of the cool, photoionized (T∼ 10 4 K) circumgalactic
medium (CGM) using the COS-Halos suite of gas column density measurements for 44 …

We use cosmological simulations from the FIRE (Feedback In Realistic Environments)
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …

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 present the grackle chemistry and cooling library for astrophysical simulations and
models. grackle provides a treatment of non-equilibrium primordial chemistry and cooling for …

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 …

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 …