Fig. 13.
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Same as Fig. 11 but for DLA system towards QSO 0528−250. This system is a proximate DLA, where the redshift difference between the quasar and the DLA corresponds to a velocity difference smaller than 5000 km s−1, i.e. c|zem − zabs|/(1 + zabs). Here we see a relatively high-velocity red-shifted component with high depletion (component 3).
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