Cosmological simulations of galaxy formation
Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …
in advancing our understanding of structure and galaxy formation in the Universe. These …
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 …
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 …
But what about...: cosmic rays, magnetic fields, conduction, and viscosity in galaxy formation
PF Hopkins, TK Chan… - Monthly Notices of …, 2020 - academic.oup.com
We present and study a large suite of high-resolution cosmological zoom-in simulations,
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …
using the FIRE-2 treatment of mechanical and radiative feedback from massive stars …
Properties of the circumgalactic medium in cosmic ray-dominated galaxy haloes
We investigate the impact of cosmic rays (CRs) on the circumgalactic medium (CGM) in
FIRE-2 simulations, for ultra-faint dwarf through Milky Way (MW)-mass haloes hosting star …
FIRE-2 simulations, for ultra-faint dwarf through Milky Way (MW)-mass haloes hosting star …
Numerical simulations of multiphase winds and fountains from star-forming galactic disks. I. Solar neighborhood TIGRESS model
CG Kim, EC Ostriker - The Astrophysical Journal, 2018 - iopscience.iop.org
Gas blown away from galactic disks by supernova (SN) feedback plays a key role in galaxy
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
evolution. We investigate outflows utilizing the solar neighborhood model of our high …
The role of magnetic fields in setting the star formation rate and the initial mass function
MR Krumholz, C Federrath - Frontiers in Astronomy and Space …, 2019 - frontiersin.org
Star-forming gas clouds are strongly magnetized, and their ionization fractions are high
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …
enough to place them close to the regime of ideal magnetohydrodyamics on all but the …
Cosmic ray feedback in the FIRE simulations: Constraining cosmic ray propagation with GeV γ-ray emission
TK Chan, D Kereš, PF Hopkins… - Monthly Notices of …, 2019 - academic.oup.com
We present the implementation and the first results of cosmic ray (CR) feedback in the
Feedback In Realistic Environments (FIRE) simulations. We investigate CR feedback in non …
Feedback In Realistic Environments (FIRE) simulations. We investigate CR feedback in non …
The impact of cosmic rays on thermal instability in the circumgalactic medium
Large reservoirs of cold (∼ 10 4 K) gas exist out to and beyond the virial radius in the
circumgalactic medium (CGM) of all types of galaxies. Photoionization modeling suggests …
circumgalactic medium (CGM) of all types of galaxies. Photoionization modeling suggests …
Cosmic ray transport in large-amplitude turbulence with small-scale field reversals
P Kempski, DB Fielding, E Quataert… - Monthly Notices of …, 2023 - academic.oup.com
The nature of cosmic ray (CR) transport in the Milky Way remains elusive. The predictions of
current microphysical CR transport models in magnetohydrodynamic (MHD) turbulence are …
current microphysical CR transport models in magnetohydrodynamic (MHD) turbulence are …