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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 …
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …
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 structure of multiphase galactic winds
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 …
galactic winds comprised of a hot, volume-filling component and a cold, clumpy component …
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
We present results from 13 cosmological simulations that explore the parameter space of the
'Evolution and Assembly of GaLaxies and their Environments'(EAGLE) simulation project …
'Evolution and Assembly of GaLaxies and their Environments'(EAGLE) simulation project …
Quasar feedback: more bang for your buck
We propose a 'two-stage'model for the effects of feedback from a bright quasar on the cold
gas in a galaxy. It is difficult for winds or other forms of feedback from near the accretion disc …
gas in a galaxy. It is difficult for winds or other forms of feedback from near the accretion disc …
The launching of cold clouds by galaxy outflows. I. Hydrodynamic interactions with radiative cooling
E Scannapieco, M Brüggen - The Astrophysical Journal, 2015 - iopscience.iop.org
To better understand the nature of the multiphase material found in outflowing galaxies, we
study the evolution of cold clouds embedded in flows of hot and fast material. Using a suite …
study the evolution of cold clouds embedded in flows of hot and fast material. Using a suite …
Driving outflows with relativistic jets and the dependence of active galactic nucleus feedback efficiency on interstellar medium inhomogeneity
We examine the detailed physics of the feedback mechanism by relativistic active galactic
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …
Hydrodynamical coupling of mass and momentum in multiphase galactic winds
EE Schneider, BE Robertson - The Astrophysical Journal, 2017 - iopscience.iop.org
Using a set of high-resolution hydrodynamical simulations run with the Cholla code, we
investigate how mass and momentum couple to the multiphase components of galactic …
investigate how mass and momentum couple to the multiphase components of galactic …
A review of the theory of galactic winds driven by stellar feedback
D Zhang - Galaxies, 2018 - mdpi.com
Galactic winds from star-forming galaxies are crucial to the process of galaxy formation and
evolution, regulating star formation, sha** the stellar mass function and the mass …
evolution, regulating star formation, sha** the stellar mass function and the mass …
Starburst-driven galactic winds: filament formation and emission processes
We have performed a series of three-dimensional simulations of the interaction of a
supersonic wind with a nonspherical radiative cloud. These simulations are motivated by our …
supersonic wind with a nonspherical radiative cloud. These simulations are motivated by our …