The infrared emission from the elliptical galaxy NGC 1052

Details The infrared emission from the elliptical galaxy NGC 1052 The infrared emission from the elliptical galaxy NGC 1052

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...263..624b&link_type=abstract

Astrophysical Journal, Part 1, vol. 263, Dec. 15, 1982, p. 624-628.

Astronomy and Astrophysics

Astronomy

27

Cosmic Dust, Elliptical Galaxies, Galactic Nuclei, Galactic Radiation, Infrared Astronomy, Astronomical Photometry, Flux Density, Shock Heating

Scientific paper

Multi-aperture IR photometry of the elliptical galaxy NGC 1052 shows
that its IR excess is confined to a region smaller than 2 arc sec (300
pc) in diameter coincident with the visible nucleus. It is suggested
that the emission in the 5-20 micron range arises from dust heated by
the nonthermal source seen at other wavelengths.

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