Theoretical challenges in galaxy formation
T Naab, JP Ostriker - Annual review of astronomy and …, 2017 - annualreviews.org
Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …
evolution. Over the decades the field has made significant progress. It is now possible to …
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical …
M Ruszkowski, C Pfrommer - The Astronomy and Astrophysics Review, 2023 - Springer
Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
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 …
Dynamical properties of z ∼4.5 dusty star-forming galaxies and their connection with local early-type galaxies
There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …
combination of stellar feedback processes and gravitational instabilities driven by mergers …
STARFORGE: Towards a comprehensive numerical model of star cluster formation and feedback
ABSTRACT We present STARFORGE (STAR FORmation in Gaseous Environments): a new
numerical framework for 3D radiation magnetohydrodynamic (MHD) simulations of star …
numerical framework for 3D radiation magnetohydrodynamic (MHD) simulations of star …
Characterizing mass, momentum, energy, and metal outflow rates of multiphase galactic winds in the FIRE-2 cosmological simulations
We characterize mass, momentum, energy, and metal outflow rates of multiphase galactic
winds in a suite of FIRE-2 cosmological 'zoom-in'simulations from the Feedback in Realistic …
winds in a suite of FIRE-2 cosmological 'zoom-in'simulations from the Feedback in Realistic …
Multiphase gas and the fractal nature of radiative turbulent mixing layers
A common situation in galactic and intergalactic gas involves cold dense gas in motion
relative to hot diffuse gas. Kelvin–Helmholtz instability creates a turbulent mixing layer and …
relative to hot diffuse gas. Kelvin–Helmholtz instability creates a turbulent mixing layer and …
SILCC VI–Multiphase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionizing radiation, and cosmic rays
TE Rathjen, T Naab, P Girichidis… - Monthly Notices of …, 2021 - academic.oup.com
We present simulations of the multiphase interstellar medium (ISM) at solar neighbourhood
conditions including thermal and non-thermal ISM processes, star cluster formation, and …
conditions including thermal and non-thermal ISM processes, star cluster formation, and …
First Results from SMAUG: Characterization of Multiphase Galactic Outflows from a Suite of Local Star-forming Galactic Disk Simulations
Large-scale outflows in star-forming galaxies are observed to be ubiquitous and are a key
aspect of theoretical modeling of galactic evolution, the focus of the Simulating Multiscale …
aspect of theoretical modeling of galactic evolution, the focus of the Simulating Multiscale …
Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
One of the key mysteries of star formation is the origin of the stellar initial mass function
(IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and …
(IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and …