Fig. 5
Determined disk abundances in this work (teal) compared with selected literature trends: Mishenina et al. (2013) (pink), Delgado Mena et al. (2017) (black), and Guiglion et al. (2018) (orange). The typical uncertainties, when available, are indicated in the lower right corner of every plot, where the uncertainties from Mishenina et al. (2013) and Delgado Mena et al. (2017) (their Tables 3 and 4, respectively) are for a low Teff star.
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