Fig. 5
Observed depletion of Zn in Galactic individual absorbers, taken from Jenkins (2009), which is the observed [Zn/H] for the Galaxy. The solid red curve shows a linear fit to the data with a slope of BδZn = −0.27 ± 0.03, which we assume for the derivation of the depletion. The dashed curve shows the expected relation from Eq. (10) of Jenkins (2009). The depletion of Zn is bound to be zero for DLAs with [Zn/Fe] = 0.
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