A unified model for the 3.28-micron emission and the 2200 A interstellar extinction feature

Details A unified model for the 3.28-micron emission and the 2200 A interstellar extinction feature A unified model for the 3.28-micron emission and the 2200 A interstellar extinction feature

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.154..143h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 154, no. 1, April 1989, p. 143-147.

Astronomy and Astrophysics

Astronomy

7

Galactic Radiation, Infrared Astronomy, Interstellar Extinction, Milky Way Galaxy, Molecular Spectra, Ultraviolet Astronomy, Diffuse Radiation, Emission Spectra, Methyl Compounds, Organic Compounds, Quinoline

Scientific paper

The 3.28-micron feature observed in the diffuse galactic emission and
the 2200 A interstellar extinction feature must have a common source.
This requirement rules out graphitic-type PAH molecules such as coronone
and tends to favor naturally occurring bicyclic ring structures typified
by quinoline and its derivatives.

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