Ariel V sky survey - Observations of X-rays from galaxies in the region of 3U 0328-52

Details Ariel V sky survey - Observations of X-rays from galaxies in the region of 3U 0328-52 Ariel V sky survey - Observations of X-rays from galaxies in the region of 3U 0328-52

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177p..21p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Oct. 1976, p. 21P-24P. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

3

Ariel 5 Satellite, Galactic Clusters, Galactic Radiation, Radiant Flux Density, Sky Surveys (Astronomy), Spaceborne Astronomy, X Ray Sources, Satellite Observation, Spatial Distribution

Scientific paper

Observations by the Ariel V sky-survey instrument in the galaxy-rich region around the X-ray source 3U 0328-52 show that the rich cluster of galaxies CA 0340-538 is probably responsible for most of the X-ray emission. For an assumed distance of 284 Mpc, this leads to an X-ray luminosity of 6.3 (+ or - 0.9) by 10 to the 44th power erg/s (2-10 keV). This result strengthens the association of X-ray emission with clusters which are rich, contain radio sources, and have dominant central galaxies.

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