Nonthermal optical-infrared emission from NGC 1052

Details Nonthermal optical-infrared emission from NGC 1052 Nonthermal optical-infrared emission from NGC 1052

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...252l..53r&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 252, Jan. 15, 1982, p. L53-L56. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

30

Bl Lacertae Objects, Galactic Nuclei, Galactic Radiation, Infrared Spectra, Nonthermal Radiation, Optical Emission Spectroscopy, Polarimetry, Stellar Luminosity, Stellar Spectrophotometry, Variability

Scientific paper

A close resemblance is noted between the IR excess spectrum of NGC 1052,
which is approximately 4.5% polarized, and the spectra of the reddest BL
Lac-type sources. Although NGC 1052 exhibits no variability, grounds are
given for the conclusion that this source is both nonthermal and of
unusually low luminosity for its type.

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