A model for superlight velocities of extragalactic radio sources

Details A model for superlight velocities of extragalactic radio sources A model for superlight velocities of extragalactic radio sources

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.265..219e&link_type=abstract

Nature, vol. 265, Jan. 20, 1977, p. 219-222. NSF-supported research.

Astronomy and Astrophysics

Astronomy

14

Astronomical Models, Extragalactic Radio Sources, Galactic Nuclei, Interstellar Gas, Light Speed, Quasars, Energy Sources, Gas Density, Relativistic Particles

Scientific paper

An explanation is proposed for apparent superlight velocities of compact radio sources. In our model high velocities are a consequence of the interaction of the radio sources with the ambient gas in a galactic nucleus or quasar. This model predicts that the pair of sources is not centered on the nucleus and that the individual components should be smaller and more separated when observed at higher frequency.

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