A 3.4 micron absorption band in amorphous carbon Implications for interstellar dust

Details A 3.4 micron absorption band in amorphous carbon Implications for interstellar dust A 3.4 micron absorption band in amorphous carbon Implications for interstellar dust

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.205p..67d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 205, Nov. 1983, p. 67P-70P. Research supported by the N

Astronomy and Astrophysics

Astronomy

63

Carbon, Cosmic Dust, Infrared Absorption, Interstellar Matter, Spectral Bands, Amorphous Materials, Chemical Bonds, Hydrocarbons

Scientific paper

The infrared absorption spectrum of hydrogenated amorphous carbon solids
shows features at 3.38, 3.41 and 3.48 μm corresponding to discrete
bands in the spectrum of IRS-7. Interstellar amorphous carbon dust with
chemisorbed CH2 and CH3 groups may be a
significant component of interstellar dust in diffuse clouds.

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