Fig. 7
Galactic warm disk depletion abundance pattern (solid line, Savage & Sembach 1996), in which Al is assumed to be depleted as strongly as Fe (Phillips et al. 1982), and depletion of O is assumed to be negligible (Jenkins 2009), fit to the observed pattern (diamonds) following Savaglio (2001). This fit yields DTM = 1.00 ± 0.01. Aluminium is not included in this fit. The limit on S is taken from Castro-Tirado et al. (2013a).
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