Fig. 10
Left: the relation between dust-to-stellar mass and HI deficiency. Right: the relation between dust-to-stellar mass and HI-to-stellar mass ratio. The dotted lines indicate constant HI-to-dust ratios of (from left to right): 30-100-300. The green lines indicate two different models of dust stripping assuming a constant (dashed) or exponential (solid) Hi surface density profile. See text for details. Symbols are as in Fig. 6.
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