Aromatic hydrocarbons in very small interstellar grains

Details Aromatic hydrocarbons in very small interstellar grains Aromatic hydrocarbons in very small interstellar grains

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.158..135w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 158, no. 1, Aug. 1989, p. 135-140.

Astronomy and Astrophysics

Astrophysics

6

Aromatic Compounds, Galactic Radiation, Hydrocarbons, Interstellar Matter, Absorption Spectra, Diffuse Radiation, Emission Spectra, Grains, Planetary Nebulae

Scientific paper

It is shown that the recently observed 3.3-micron emission feature in
the diffuse radiation from the galactic disk might be due to an ensemble
of aromatic molecules distributed within very small interstellar grains.
The same particles also provide an explanation of the 2200 A
interstellar absorption feature.

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