Fig. 4
Depletion factor, [X/Zn], of different species relative to zinc calculated by integrating the column densities over the whole profile. Dotted, dashed, and solid lines correspond to depletion factors observed in, respectively, the halo, the warm, and cold ISM of the Galaxy (Welty et al. 1999). Note that the depletion factor observed in the Galaxy for copper is unavailable.
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