Radio and X-ray observations of the Abell 2241 galaxy clusters

Details Radio and X-ray observations of the Abell 2241 galaxy clusters Radio and X-ray observations of the Abell 2241 galaxy clusters

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...111...50b&link_type=abstract

Astronomy and Astrophysics, vol. 111, no. 1, July 1982, p. 50-57. Research supported by the Nederlandse Organisatie voor Zuiver

Astronomy and Astrophysics

Astronomy

13

Astronomical Maps, Galactic Clusters, Radio Astronomy, X Ray Sources, Galactic Structure, Intergalactic Media, Radio Galaxies, Red Shift

Scientific paper

Radio and X-ray observations of the two independent clusters in the A 2241 region are presented. The difference in both the radio and the X-ray behavior between the dominant galaxies of the two clusters is interpreted as being due to different densities of the intra cluster medium. In the most distant cluster evidence is found for a large gaseous halo surrounding the central galaxy, which by buoyant forces also influences the shape of the 420 kpc long head-tail galaxy.

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