Detection of the 3.3 micron feature in the Seyfert galaxy NGC 4151

Details Detection of the 3.3 micron feature in the Seyfert galaxy NGC 4151 Detection of the 3.3 micron feature in the Seyfert galaxy NGC 4151

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241l.141c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 241, Nov. 1, 1980, p. L141-L144.

Astronomy and Astrophysics

Astronomy

22

Galactic Radiation, Infrared Astronomy, Infrared Spectra, Seyfert Galaxies, Cosmic Dust, Near Infrared Radiation, Thermal Radiation

Scientific paper

The emission feature at 3.3 micron has been detected in the
near-infrared spectrum of the Seyfert galaxy NGC 4151. Although not yet
identified, this feature is seen in many galactic thermal sources, and
its presence suggests that at least a large fraction of the infrared
emission in NGC 4151 is due to thermal radiation by dust.

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