John ZuHone

TL;DR: In this paper, the authors used high-resolution N-body/Eulerian hydrodynamic simulations to study gas sloshing in galaxy clusters initiated by mergers with subclusters.

TL;DR: In this paper, high-resolution magnetohydrodynamics simulations of magnetized gas sloshing in galaxy clusters initiated by encounters with subclusters have been performed, where strong velocity shears associated with the cold fronts are observed to amplify the magnetic field along the cold front surfaces, increasing magnetic field strength in these layers by up to an order of magnitude.

TL;DR: In this paper, a high-resolution MHD simulation of gas sloshing in a galaxy cluster coupled with subgrid simulations of relativistic electron acceleration is presented to test this hypothesis.

TL;DR: The Lynx architecture enables a broad range of unique and compelling science to be carried out mainly through a General Observer Program, envisioned to include detecting the very first seed black holes, revealing the high-energy drivers of galaxy formation and evolution, and characterizing the mechanisms that govern stellar evolution and stellar ecosystems.

TL;DR: The ASTRO-H mission as mentioned in this paper is equipped with a suite of sensitive instruments with the highest energy resolution ever achieved at E > 3 keV and a wide energy range spanning four decades in energy from soft X-rays to gamma-rays.