The infrared spectrum of NGC 1068

Details The infrared spectrum of NGC 1068 The infrared spectrum of NGC 1068

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199l..13r&link_type=abstract

Astrophysical Journal, vol. 199, July 1, 1975, pt. 2, p. L13-L17. NSF-supported research.

Astronomy and Astrophysics

Astronomy

70

Astronomical Photometry, Galactic Nuclei, Galactic Radiation, Infrared Astronomy, Infrared Spectra, Absorption Spectra, Cosmic Dust, Luminous Intensity, Spectral Energy Distribution

Scientific paper

New infrared photometry of NGC 1068 shows that the spectrum continues to rise smoothly through 34 microns and that there is a shallow absorption feature near 10 microns. The total infrared flux from the nuclear source is about 2.3 times 10 to the minus 11th watts per sq m, which corresponds to a luminosity of 10 to the 11th suns at a distance of 11 Mpc.

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