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A qualitatively new model of patchy CR scattering
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First Constraints on CR Transport in CGM
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CRs can explain multiphase kinematic alignment
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CRs qualitatively alter cold CGM gas that forms through thermal instability
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CGM structure is incredibly sensitive to choice of CR transport
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Ultraviolet observations of galaxy cluster outskirts unlock structure invisible to X-rays
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Supernovae Can Seed Galactic Magnetic Fields
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Baryons alter dark matter distributions in galaxy simulations
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QPOs in Accretion Disks Could be Caused by Corrugation Modes