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 …
from cosmological to subparsec scales, the past decade has seen major theoretical …
The structure of multiphase galactic winds
DB Fielding, GL Bryan - The Astrophysical Journal, 2022 - iopscience.iop.org
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 …
Pressure-regulated, Feedback-modulated Star Formation in Disk Galaxies
EC Ostriker, CG Kim - The Astrophysical Journal, 2022 - iopscience.iop.org
The star formation rate (SFR) in galactic disks depends on both the quantity of the available
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …
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 …
FIREbox: simulating galaxies at high dynamic range in a cosmological volume
R Feldmann, E Quataert… - Monthly Notices of …, 2023 - academic.oup.com
We introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …
Star formation efficiency and dispersal of giant molecular clouds with UV radiation feedback: dependence on gravitational boundedness and magnetic fields
JG Kim, EC Ostriker, N Filippova - The Astrophysical Journal, 2021 - iopscience.iop.org
Molecular clouds are supported by turbulence and magnetic fields, but quantifying their
influence on cloud life cycle and star formation efficiency (SFE) remains an open question …
influence on cloud life cycle and star formation efficiency (SFE) remains an open question …
JWST reveals widespread AGN-driven neutral gas outflows in massive z ~ 2 galaxies
We use deep JWST/NIRSpec R∼ 1000 slit spectra of 113 galaxies at, selected from the
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …
mass-complete Blue Jay survey, to investigate the prevalence and typical properties of …
Theory and Observation of Winds from Star-Forming Galaxies
TA Thompson, TM Heckman - Annual Review of Astronomy and …, 2024 - annualreviews.org
Galactic winds shape the stellar, gas, and metal content of galaxies. To quantify their impact,
we must understand their physics. We review potential wind-driving mechanisms and …
we must understand their physics. We review potential wind-driving mechanisms and …
Cosmological simulations of quasar fueling to subparsec scales using lagrangian hyper-refinement
D Anglés-Alcázar, E Quataert, PF Hopkins… - The Astrophysical …, 2021 - iopscience.iop.org
We present cosmological hydrodynamic simulations of a quasar-mass halo (M halo≈ 10
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …
12.5 M⊙ at z= 2) that for the first time resolve gas transport down to the inner 0.1 pc …
SILCC–VII. Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
TE Rathjen, T Naab, S Walch, D Seifried… - Monthly Notices of …, 2023 - academic.oup.com
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase
interstellar medium (ISM) in stratified galactic patches with gas surface densities Σgas= 10 …
interstellar medium (ISM) in stratified galactic patches with gas surface densities Σgas= 10 …