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Fig. 8.

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Ratio of the fraction of baryons (left panel) and cold gas (right panel) in a shell between r hm $ r^{\star}_{\mathrm{hm}} $ and 0.15 r200 to those within r hm $ r^{\star}_{\mathrm{hm}} $, as a function of stellar mass. References are as in Fig. 7. Dotted horizontal lines mark unit ratios.

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