Illustrative elemental abundances and depletions for dust-forming elements in the diffuse ISM, based upon the THEMIS dust model (Jones et al. 2017).
Notes. The possible range of O abundances are indicated (490:575, Asplund et al. 2009; Przybilla et al. 2008, respectively). The C abundance is taken from Jenkins (2009) and Parvathi et al. (2012). Otherwise the abundances are from Jenkins (2009) and Palme et al. (2014). As explained in the text, ~ 10% of O and N heteroatoms, relative to carbon, has been included within a-C(:H) mantles.
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