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. Author manuscript; available in PMC: 2018 Jul 4.
Published in final edited form as: Plasma Sources Sci Technol. 2018 Mar 14;27:035007. doi: 10.1088/1361-6595/aab185

Figure 1.

Figure 1

Upper panel: approximate a-C:H structure for the predominant component of interstellar dust based on the model suggested by Dartois et al. [9] Lower panel: Comparison of the theoretical IR spectrum for the structure in the upper panel with that of a typical a-C:H sample (thickness ≈570 nm) deposited in the present work.