Morphology and peculiar velocities of radio sources in rich clusters of galaxies

Details Morphology and peculiar velocities of radio sources in rich clusters of galaxies Morphology and peculiar velocities of radio sources in rich clusters of galaxies

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..221g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, July 1978, p. 221-225. Research supported by the National Research

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Galactic Clusters, Radial Velocity, Radio Sources (Astronomy), Astrodynamics, Morphology, Red Shift, Velocity Measurement

Scientific paper

We examine data pertinent to a test for correlation between the peculiar velocities and the radio morphologies of radio sources in rich clusters of galaxies. The significance of the test is presently limited by the small amount of data on 'classical double' and 'wide tail' structures in rich clusters, but models wherein distortions from the 'classical double' form increase with the peculiar velocity of the parent galaxy are marginally favored.

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