Beamed radio and far infrared emission in quasars and radio galaxies.

Details Beamed radio and far infrared emission in quasars and radio galaxies. Beamed radio and far infrared emission in quasars and radio galaxies.

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...319..757h&link_type=abstract

Astronomy and Astrophysics, v.319, p.757-763

Astronomy and Astrophysics

Astrophysics

20

Galaxies: Active, Galaxies: Jets, Quasars: General, Infrared: Galaxies

Scientific paper

Simple orientation model predictions for the radio to far infrared spectral energy distributions of radio-loud AGN are confronted with observations at various radio frequencies. This model is subsequently used to investigate 60μm far-infrared data. The results are supportive of the unified scheme for Fanaroff-Riley class II radio galaxies and quasars. The relative strength of the beamed component is derived as a function of frequency, and it is found that the higher far infrared fluxes of quasars, as compared to radio galaxies, can be explained invoking moderately beamed nonthermal far-infrared emission.

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