Energy distributions of radio galaxies

Details Energy distributions of radio galaxies Energy distributions of radio galaxies

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....105..853i&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 105, no. 3, p. 853-863.

Astronomy and Astrophysics

Astronomy

36

Energy Distribution, Infrared Astronomy Satellite, Infrared Radiation, Luminous Intensity, Radio Galaxies, Red Shift, Astronomical Catalogs, Far Infrared Radiation, Spectrum Analysis

Scientific paper

Far-infrared observations of 140 radio galaxies which span a range of over four orders of magnitude in radio power, (from weak nuclear sources in nearby galaxies, to powerful FR II doubled lobed sources at moderate redshift) are presented. The strength of the far-infrared emission is more closely correlated with core than total radio emission. Far-infrared emission in radio galaxies represents star formation that is more closely tied to the active nucleus than to the global properties of the galaxy. The far-infrared luminosity function shows good continuity between radio galaxies and radio loud quasars.

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