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. Author manuscript; available in PMC: 2020 Aug 3.
Published in final edited form as: Astrophys J. 2016 Jul 12;825(2):136. doi: 10.3847/0004-637x/825/2/136

Figure 3.

Figure 3.

The calculated fraction, fdust(X) of the total abundance of X = {Mg, Si, Fe} that is locked up in thermally-condensed dust (grey bars), is compared to observed values in the cool (blue) and hot (red) phases of the interstellar medium (Savage & Sembach 1996).