On the distribution of radio emission in the X-ray cluster of galaxies Abell 401

Details On the distribution of radio emission in the X-ray cluster of galaxies Abell 401 On the distribution of radio emission in the X-ray cluster of galaxies Abell 401

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85..773b&link_type=abstract

Astronomical Journal, vol. 85, July 1980, p. 773-779.

Astronomy and Astrophysics

Astronomy

17

Galactic Clusters, Galactic Radio Waves, Radio Astronomy, Radio Galaxies, X Ray Sources, Astronomical Maps, Galactic Structure, Polarization (Waves), Very Large Array (Vla)

Scientific paper

The study deals with 4885-MHz very large array (VLA) observations of four galaxies in the rich cluster Abell 401. High-resolution VLA maps reveal several new features in the radio galaxies, e.g., 4C13.17A is unusually highly polarized near the galaxy nucleus unlike other head-tail sources. 4C13.17B is shown for the first time to have characteristics similar to the U-shaped source NGC 1265. From these maps models are produced that required the hot ICM that has been detected by X-ray observations. It is noted that there should be a correlation between the radio and X-ray emission from massive galaxies in clusters.

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