63 citations · 372 across the 15 of their papers we have counts for
15 papers
Deep Learning Cosmic Ray Transport from Density Maps of Simulated, Turbulent Gas
Chad Bustard, John Wu
The coarse-grained propagation of Galactic cosmic rays (CRs) is traditionally constrained by phenomenological models of Milky Way CR propagation fit to a variety of direct and indi…
Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
Yong Zheng, Kirill Tchernyshyov, Knut Olsen +11
The Large Magellanic Cloud (LMC) is home to many HII regions, which may lead to significant outflows. We examine the LMC's multiphase gas ( K) in HI, SII, SiIV, and…
The Impact of Cosmic Rays on Thermal and Hydrostatic Stability in Galactic Halos
Tsun Hin Navin Tsung, S. Peng Oh, Chad Bustard
We investigate how cosmic rays (CRs) affect thermal and hydrostatic stability of circumgalactic (CGM) gas, in simulations with both CR streaming and diffusion. Local thermal instab…
Cosmic Ray Drag and Damping of Compressive Turbulence
Chad Bustard, S. Peng Oh
While it is well-known that cosmic rays (CRs) can gain energy from turbulence via second order Fermi acceleration, how this energy transfer affects the turbulent cascade remains la…
Turbulent Reacceleration of Streaming Cosmic Rays
Chad Bustard, S. Peng Oh
Subsonic, compressive turbulence transfers energy to cosmic rays (CRs), a process known as non-resonant reacceleration. It is often invoked to explain observed ratios of primary to…
Radiative Turbulent Mixing Layers and the Survival of Magellanic Debris
Chad Bustard, Max Gronke
The Magellanic Stream is sculpted by its infall through the Milky Way's circumgalactic medium, but the rates and directions of mass, momentum, and energy exchange through the Strea…