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 …

Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges

RA Crain, F van de Voort - Annual Review of Astronomy and …, 2023 - annualreviews.org
We review the progress in modeling the galaxy population in hydrodynamical simulations of
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …

Introducing the thesan project: radiation-magnetohydrodynamic simulations of the epoch of reionization

R Kannan, E Garaldi, A Smith, R Pakmor… - Monthly Notices of …, 2022 - academic.oup.com
We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

The IllustrisTNG simulations: public data release

D Nelson, V Springel, A Pillepich… - Computational …, 2019 - Springer
We present the full public release of all data from the TNG100 and TNG300 simulations of
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …

First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback

D Nelson, A Pillepich, V Springel… - Monthly Notices of …, 2019 - academic.oup.com
We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …

First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time

A Pillepich, D Nelson, V Springel… - Monthly Notices of …, 2019 - academic.oup.com
We present a new cosmological, magnetohydrodynamical simulation for galaxy formation:
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

A Pillepich, D Nelson, L Hernquist… - Monthly Notices of …, 2018 - academic.oup.com
The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations
of galaxy formation performed with the arepo code and updated models for feedback …

The MillenniumTNG project: the galaxy population at z ≥ 8

R Kannan, V Springel, L Hernquist… - Monthly Notices of …, 2023 - academic.oup.com
The early release science results from JWST have yielded an unexpected abundance of
high-redshift luminous galaxies that seems to be in tension with current theories of galaxy …

The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations

V Rodriguez-Gomez, GF Snyder, JM Lotz… - Monthly Notices of …, 2019 - academic.oup.com
We have generated synthetic images of∼ 27 000 galaxies from the IllustrisTNG and the
original Illustris hydrodynamic cosmological simulations, designed to match Pan-STARRS …

The redshift evolution of the binary black hole merger rate: A weighty matter

LAC Van Son, SE De Mink, T Callister… - The Astrophysical …, 2022 - iopscience.iop.org
Gravitational-wave detectors are starting to reveal the redshift evolution of the binary black
hole (BBH) merger rate, R BBH (z). We make predictions for R BBH (z) as a function of black …