Very broad-band structure and emission by hydrogenated amorphous carbon

Details Very broad-band structure and emission by hydrogenated amorphous carbon Very broad-band structure and emission by hydrogenated amorphous carbon

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242p..40d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 15, 1990, p. 40P-42P. Research supported by N

Astronomy and Astrophysics

Astronomy

10

Carbon, Interstellar Extinction, Molecular Clouds, Amorphous Materials, Broadband, Interstellar Chemistry, Interstellar Matter

Scientific paper

New laboratory data show that an efficient broad-band luminescence is emitted by hydrogenated amorphous carbon (HAC) solids with large hydrogen content. The peak wavelength and spectral extent of this emission closely coincides with the wavelength dependence of the very broad structure (VBS). It is suggested that a polymeric form of HAC may be present in diffuse clouds. Emission from this material should be observable in the spectrum of the diffuse galactic light.

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