2 papers
astro-ph.GA2025
Development of Turbulence in Post-shock Regions
Michael M. Foley, Philip Mocz, Blakesley Burkhart +2
Supersonic isothermal turbulence is ubiquitous in the interstellar medium. This work presents high-resolution AREPO hydrodynamical simulations of isolated shocks moving through sup…
astro-ph.GA2024
Tracing 3-D Magnetic Field Structure Using Dust Polarization and the Zeeman Effect
Brandon Shane, Blakesley Burkhart, Laura Fissel +3
The characterization of magnetic fields within molecular clouds is fundamental to understanding star formation processes. Accurately gauging the three-dimensional structure of thes…