Measurements of galactic nuclei at 34 microns

Details Measurements of galactic nuclei at 34 microns Measurements of galactic nuclei at 34 microns

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200l..67r&link_type=abstract

Astrophysical Journal, vol. 200, Sept. 1, 1975, pt. 2, p. L67-L69. NSF-supported research.

Astronomy and Astrophysics

Astronomy

64

Far Infrared Radiation, Galactic Nuclei, Infrared Astronomy, Luminous Intensity, Angular Resolution, Atmospheric Windows, Emission Spectra, Infrared Spectra, Line Spectra, Power Spectra, Radiation Measurement, Seyfert Galaxies, Telescopes

Scientific paper

Results are reported for IR observations of the nuclei of NGC 1275, NGC 4151, Markarian 231, NGC 5195, and NGC 5253 which were made at 34 microns with the NASA 61-inch telescope. The total luminosity of these sources is estimated, and it is found that the total luminosity of Markarian 231 is nearly 10 trillion times that of the sun. It is noted that this power output lies within the luminosity range of quasars.

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