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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 …
Impact of low-energy cosmic rays on star formation
In recent years, exciting developments have taken place in the identification of the role of
cosmic rays in star-forming environments. Observations from radio to infrared wavelengths …
cosmic rays in star-forming environments. Observations from radio to infrared wavelengths …
Star formation near the Sun is driven by expansion of the Local Bubble
For decades we have known that the Sun lies within the Local Bubble, a cavity of low-
density, high-temperature plasma surrounded by a shell of cold, neutral gas and dust …
density, high-temperature plasma surrounded by a shell of cold, neutral gas and dust …
The synchrony of production and escape: half the bright Lyα emitters at z ≈ 2 have Lyman continuum escape fractions ≈50
The ionizing photon escape fraction [Lyman continuum (LyC) f esc] of star-forming galaxies
is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit …
is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit …
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 …
Efficiently Cooled Stellar Wind Bubbles in Turbulent Clouds. I. Fractal Theory and Application to Star-forming Clouds
Winds from massive stars have velocities of 1000 km s− 1 or more and produce hot, high-
pressure gas when they shock. We develop a theory for the evolution of bubbles driven by …
pressure gas when they shock. We develop a theory for the evolution of bubbles driven by …
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 …
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 …
Introducing TIGRESS-NCR. I. Coregulation of the Multiphase Interstellar Medium and Star Formation Rates
Massive, young stars are the main source of energy that maintains multiphase structure and
turbulence in the interstellar medium (ISM), and without this" feedback" the star formation …
turbulence in the interstellar medium (ISM), and without this" feedback" the star formation …
Efficiently cooled stellar wind bubbles in turbulent clouds. ii. validation of theory with hydrodynamic simulations
In a companion paper, we develop a theory for the evolution of stellar wind-driven bubbles
in dense, turbulent clouds. This theory proposes that turbulent mixing at a fractal …
in dense, turbulent clouds. This theory proposes that turbulent mixing at a fractal …