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Fig. 14.

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Mass in-flux (top panel), cloud surface area (center), and mean interface density (lower) as a function of radius for clouds in the inner halo (galactocentric distance ∼0.3 R200c). The various solid colored curves correspond to median relations for clouds segregated into different mass bins, scatter points to individual clouds, and the dashed gray lines to relevant scaling relations. See main text for more discussion.

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