IRAS observations of NGC 1052

Details IRAS observations of NGC 1052 IRAS observations of NGC 1052

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..973n&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, Dec. 1984, p. 973-976.

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Elliptical Galaxies, Infrared Astronomy Satellite, Spaceborne Astronomy, Cosmic Dust, Emission Spectra, Galactic Nuclei, Infrared Spectra, Spectral Energy Distribution, Thermal Radiation

Scientific paper

The galaxy NGC 1052 has been observed with the IRAS satellite. The infrared emission at 100 microns is substantially larger than a smooth extrapolation of the radio data. Because of the large diaphragm size of IRAS, it is impossible to decide uniquely if the infrared radiation represents a self-absorbed nonthermal spectrum or thermal reradiation by heated dust.

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