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Atomic Chemistry in Turbulent Astrophysical Media II: Effect of the Redshift Zero Metagalactic Background
William J Gray, Evan Scannapieco
We carry out direct numerical simulations of turbulent astrophysical media exposed to the redshift zero metagalactic background. The simulations assume solar composition and explic…
"Observing and Analyzing" Images From a Simulated High Redshift Universe
Robert J. Morgan, Rogier A. Windhorst, Evan Scannapieco +1
We investigate the high-redshift evolution of the restframe UV-luminosity function (LF) of galaxies via hydrodynamical cosmological simulations, coupled with an emulated observatio…
The Launching of Cold Clouds by Galaxy Outflows I: Hydrodynamic Interactions with Radiative Cooling
Evan Scannapieco, Marcus Brüggen
To better understand the nature of the multiphase material found in outflowing galaxies, we study the evolution of cold clouds embedded in flows of hot and fast material. Using a s…
Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic Cooling
William J Gray, Evan Scannapieco, Daniel Kasen
We carry out direct numerical simulations of turbulent astrophysical media that explicitly track ionizations, recombinations, and species-by-species radiative cooling. The simulati…