X-ray and radio observations of the structure of Abell 478

Details X-ray and radio observations of the structure of Abell 478 X-ray and radio observations of the structure of Abell 478

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...217l..15s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 217, Oct. 1, 1977, p. L15-L18.

Astronomy and Astrophysics

Astronomy

14

Galactic Clusters, Radio Galaxies, Sas, X Ray Sources, Galactic Structure, Radio Sources (Astronomy), Spaceborne Astronomy

Scientific paper

The complex X-ray and radio structures of the cluster of galaxies Abell 478 have been observed in the 2-11-keV energy band by the rotating modulation collimators on the SAS-3 X-ray observatory and at 1415 MHz by the Westerbork synthesis radio telescope. The X-ray data imply an extended source (X-ray luminosity of the order of 10 to the 45th power erg/s) and are consistent with the presence of a coincident pointlike source X-ray luminosity of the order of 10 to the 45th power erg/s. The X-ray source position is also coincident with a cD radio galaxy at the core of the cluster.

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