A search for X-ray emission associated with the great attractor

Astronomy and Astrophysics – Astronomy

Scientific paper

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Emission Spectra, Galactic Clusters, Intergalactic Media, Sky Surveys (Astronomy), X Ray Sources, Active Galaxies, Brightness Distribution, Density Distribution, Diffuse Radiation, High Temperature Gases

Scientific paper

A search is reported for X-ray emission associated with the object, dubbed the 'great attractor', which has been postulated as the cause of the coherent deviations from the Hubble flow which are observed in nearby parts of the universe. The hypothesis that a substantial fraction of the dynamical mass of the great attractor exists in the form of rich clusters of galaxies is ruled out. The possibility is considered that a substantial fraction of the mass of the great attractor could exist in a form which would increase the apparently diffuse X-ray surface brightness. The observational upper limit to the diffuse X-ray sky surface brightness enhancement in the general direction of the great attractor allows interesting limits to be set on the fraction of the dynamical mass of the great attractor which can exist in the form of X-ray-luminous material.

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