Modeling the cool CGM as ~10^3 misty cloud complexes of radius ~10 kpc matches MgII absorption data, and the product of average column density and covering fraction yields a robust cool gas mass estimate.
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Misty, patchy, and turbulent: constraining the cool circumgalactic medium with mCC
Modeling the cool CGM as ~10^3 misty cloud complexes of radius ~10 kpc matches MgII absorption data, and the product of average column density and covering fraction yields a robust cool gas mass estimate.