Fig. 2.
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Vertical surface densities projected through the galactic disks and inner CGM of both the CRMHD (left) and the MHD (right) simulations at t = 1 Gyr. Stellar feedback and CRs lift significantly more gas mass above the CRMHD disk than the much weaker galactic wind originating from the MHD galaxy, which lacks the additional support by CRs.
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