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Key physical processes in the circumgalactic medium
CA Faucher-Giguère, SP Oh - Annual Review of Astronomy and …, 2023 - annualreviews.org
Spurred by rich, multiwavelength observations and enabled by new simulations, ranging
from cosmological to subparsec scales, the past decade has seen major theoretical …
from cosmological to subparsec scales, the past decade has seen major theoretical …
The circumgalactic medium
J Tumlinson, MS Peeples… - Annual Review of …, 2017 - annualreviews.org
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 …
radii is known as the circumgalactic medium (CGM). In recent years this component of …
simba: Cosmological simulations with black hole growth and feedback
We introduce the simba simulations, the next generation of the mufasa cosmological galaxy
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …
First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback
We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …
The MOSDEF Survey: The Evolution of the Mass–Metallicity Relation from z= 0 to z∼ 3.3
We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z= 0–3.3
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …
FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations
Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky
Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we …
Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we …
FIRE-2 simulations: physics versus numerics in galaxy formation
ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …
What causes the formation of discs and end of bursty star formation?
As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
Cool outflows in galaxies and their implications
Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations
D Anglés-Alcázar, CA Faucher-Giguère… - Monthly Notices of …, 2017 - academic.oup.com
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 …
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …