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In a new paper (Buie II et al. 2022, ApJ, in press), we extend our previous CGM models to include angular momentum and MHD
This short video gives a quick overview of a few results from our most recent paper [1] on photoionized turbulent gas in the circumgalactic medium (CGM). The paper is the third in a series on simulations of photoionized turbulence. [2] [3] We find rotation in the halo promotes additional cooling, as it encourages mixing between hot and cool material, while the magnetic field assists with angular momentum transfer throughout the cool gas.