559 citations · 2.6k across the 23 of their papers we have counts for
13 papers · 1 filter
Highly-mass-loaded hot galactic winds are unstable to cool filament formation
Dustin D. Nguyen, Todd A. Thompson, Evan E. Schneider +1
When cool clouds are ram-pressure accelerated by a hot supersonic galactic wind, some of the clouds may be shredded by hydrodynamical instabilities and incorporated into the hot fl…
Dynamics of hot galactic winds launched from spherically-stratified starburst cores
Dustin D. Nguyen, Todd A. Thompson, Evan E. Schneider +2
The analytic galactic wind model derived by Chevalier and Clegg in 1985 (CC85) assumes energy and mass-injection within the starburst galaxy nucleus. However, th…
Revealing the Galaxy-Halo Connection Through Machine Learning
Ryan Hausen, Brant E. Robertson, Hanjue Zhu +5
Understanding the connections between galaxy stellar mass, star formation rate, and dark matter halo mass represents a key goal of the theory of galaxy formation. Cosmological simu…
Simulated Observations of Multiphase Galactic Winds
Lita M. de la Cruz, Evan E. Schneider, Eve C. Ostriker
Supernova-driven galactic winds are multiphase streams of gas that are often observed flowing at a range of velocities out of star-forming regions in galaxies. In this study, we us…
The Characteristic Momentum of Radiatively Cooling Energy-Driven Galactic Winds
Cassandra Lochhaas, Todd A. Thompson, Evan E. Schneider
Energy injection by supernovae may drive hot supersonic galactic winds in rapidly star-forming galaxies, driving metal-enriched gas into the circumgalactic medium and potentially a…
First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
Drummond B. Fielding, Stephanie Tonnesen, Daniel DeFelippis +12
We examine the properties of the circumgalactic medium (CGM) at low redshift in a range of simulated Milky Way mass halos. The sample is comprised of seven idealized simulations, a…
The Physical Nature of Starburst-Driven Galactic Outflows
Evan E. Schneider, Eve C. Ostriker, Brant E. Robertson +1
We present the fourth of the Cholla Galactic OutfLow Simulations suite (CGOLS). Using a physically-motivated prescription for clustered supernova feedback, we successfully drive a…
Infrared Galaxies in the Field of the Massive Cluster Abell S1063: Discovery of a Luminous Kiloparsec-Sized HII Region in a Gravitationally Lensed IR-Luminous Galaxy at
Gregory L. Walth, Eiichi Egami, Benjamin Clément +10
Using the Spitzer Space Telescope and Herschel Space Observatory, we have conducted a survey of infrared galaxies in the field of the galaxy cluster Abell S1063 (AS1063) at $z=0.34…
Astro2020 Science White Paper: Cold Gas Outflows, Feedback, and the Shaping of Galaxies
Alberto D. Bolatto, Lee Armus, Sylvain Veilleux +12
There is wide consensus that galaxy outflows are one of the most important processes determining the evolution of galaxies through cosmic time, for example playing a key role in sh…
Galaxy Winds in the Age of Hyperdimensional Astrophysics
Grant R. Tremblay, Evan E. Schneider, Alexey Vikhlinin +9
The past decade began with the first light of ALMA and will end at the start of the new era of hyperdimensional astrophysics. Our community-wide movement toward highly multiwavelen…
Introducing CGOLS: The Cholla Galactic OutfLow Simulation Suite
Evan E. Schneider, Brant E. Robertson
We present the Cholla Galactic OutfLow Simulations (CGOLS) suite, a set of extremely high resolution global simulations of isolated disk galaxies designed to clarify the nature of…
Production of Cool Gas in Thermally-Driven Outflows
Evan E. Schneider, Brant E. Robertson, Todd A. Thompson
Galactic outflows commonly contain multiphase gas, and its physical origin requires explanation. Using the CGOLS (Cholla Galactic OutfLow Simulations) suite of high-resolution isol…
Hydrodynamical Coupling of Mass and Momentum in Multiphase Galactic Winds
Evan E. Schneider, Brant E. Robertson
Using a set of high resolution hydrodynamical simulations run with the Cholla code, we investigate how mass and momentum couple to the multiphase components of galactic winds. The…