On the possible non-isotropy of the radio emission from compact extragalactic objects

Details On the possible non-isotropy of the radio emission from compact extragalactic objects On the possible non-isotropy of the radio emission from compact extragalactic objects

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980phys...21..662r&link_type=abstract

(University of Copenhagen, Danish Research Council and Nordisk Institut for Teoretisk Atomfysik, Copenhagen Symposium on the Uni

Astronomy and Astrophysics

Astronomy

5

Anisotropy, Astronomical Models, Extragalactic Radio Sources, Radio Emission, Mapping, Quasars, Very Long Base Interferometry

Scientific paper

A simple model is described which gives a natural explanation of the major physical differences between the two main classes of extragalactic radio sources. The model also accounts for the observed ratio of radio-quiet to radio quasars. If this model is correct the dominant radio emission from about half the detected extragalactic objects is highly anisotropic.

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