The cosmic baryon and metal cycles
C Péroux, JC Howk - Annual Review of Astronomy and …, 2020 - annualreviews.org
Characterizing the relationship between stars, gas, and metals in galaxies is a critical
component of understanding the cosmic baryon cycle. We compile contemporary censuses …
component of understanding the cosmic baryon cycle. We compile contemporary censuses …
WALLABY – an SKA Pathfinder H i survey
Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …
Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
M Donnari, A Pillepich, GD Joshi… - Monthly Notices of …, 2021 - academic.oup.com
We use the IllustrisTNG hydrodynamical simulations to show how the fractions of quenched
galaxies vary across different environments and cosmic time, and to quantify the role AGN …
galaxies vary across different environments and cosmic time, and to quantify the role AGN …
Resolving small-scale cold circumgalactic gas in TNG50
We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to
explore the properties and origin of cold circumgalactic medium (CGM) gas around massive …
explore the properties and origin of cold circumgalactic medium (CGM) gas around massive …
Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
Negative feedback from active galactic nuclei (AGN) is the leading mechanism for the
quenching of massive galaxies in the vast majority of modern galaxy evolution models …
quenching of massive galaxies in the vast majority of modern galaxy evolution models …
Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
Using the IllustrisTNG simulations, we investigate the connection between galaxy
morphology and star formation in central galaxies with stellar masses in the range 109 …
morphology and star formation in central galaxies with stellar masses in the range 109 …
Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations
We compare the star-forming main sequence (SFMS) of galaxies–both integrated and
resolved on 1 kpc scales–between the high-resolution TNG50 simulation of IllustrisTNG and …
resolved on 1 kpc scales–between the high-resolution TNG50 simulation of IllustrisTNG and …
Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
We explore three sets of cosmological hydrodynamical simulations, IllustrisTNG (TNG50,
TNG100, and TNG300), EAGLE, and SIMBA, to investigate the physical processes impacting …
TNG100, and TNG300), EAGLE, and SIMBA, to investigate the physical processes impacting …
Galaxy cold gas contents in modern cosmological hydrodynamic simulations
We present a comparison of galaxy atomic and molecular gas properties in three recent
cosmological hydrodynamic simulations, namely SIMBA, EAGLE, and IllustrisTNG, versus …
cosmological hydrodynamic simulations, namely SIMBA, EAGLE, and IllustrisTNG, versus …
Interacting galaxies in the IllustrisTNG simulations–II: star formation in the post-merger stage
MH Hani, H Gosain, SL Ellison… - Monthly Notices of the …, 2020 - academic.oup.com
Galaxy mergers are a major evolutionary transformation whose effects are borne out by a
plethora of observations and numerical simulations. However, most previous simulations …
plethora of observations and numerical simulations. However, most previous simulations …