Chemical Groups in Hydrogenated Amorphous Carbon and the Interstellar Infrared Emission Features

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ID: 317063
2026
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Abstract
Abstract Surface enhanced Raman spectroscopy (SERS) has been used to probe the molecular structure of hydrogenated amorphous carbon (a-C: H or HAC) nanoparticles. Using the known aromatic infrared bands (AIBs) as a template for comparison with SERS spectra, it is apparent that many of the molecular groups that produce these bands as well as the carbonaceous absorption bands in the diffuse interstellar medium are present in a-C: H nanoparticles. As these particles are thought to decompose through the elimination of a limited range of relatively small molecules when exposed to intense ultraviolet radiation, these data support a model in which the AIB emission can be associated with molecular fragments created during the dissolution of a-C: H nanoparticles.
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openalex_W7164383666 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors W W Duley
Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1083
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