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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 …
Atomic hydrogen in the milky way: a step** stone in the evolution of galaxies
Atomic hydrogen (Hi) is a critical step** stone in the gas evolution cycle of the interstellar
medium (ISM) of the Milky Way. Hi traces both the cold, premolecular state before star …
medium (ISM) of the Milky Way. Hi traces both the cold, premolecular state before star …
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 …
Pressure-regulated, feedback-modulated star formation in disk galaxies
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 …
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 …
Dynamical equilibrium in the molecular ISM in 28 nearby star-forming galaxies
We compare the observed turbulent pressure in molecular gas, P turb, to the required
pressure for the interstellar gas to stay in equilibrium in the gravitational potential of a …
pressure for the interstellar gas to stay in equilibrium in the gravitational potential of a …
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 …
The physical nature of starburst-driven galactic outflows
We present the fourth simulation of the Cholla Galactic OutfLow Simulations suite. Using a
physically motivated prescription for clustered supernova feedback, we successfully drive a …
physically motivated prescription for clustered supernova feedback, we successfully drive a …