The spatial distribution of X-ray clusters of galaxies

Details The spatial distribution of X-ray clusters of galaxies The spatial distribution of X-ray clusters of galaxies

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.238..881l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 238, May 15, 1989, p. 881-895. Research supported by th

Astronomy and Astrophysics

Astronomy

145

Galactic Clusters, X Ray Astronomy, Cosmology, Dipole Moments, Infrared Astronomy Satellite, Milky Way Galaxy, Spatial Distribution

Scientific paper

A reasonably complete all-sky sample of the 53 X-ray brightest clusters of galaxies is presented. A high frequency of pairs is noted, along with an exceptional concentration in the direction of the 'Great Attractor', but at a much larger distance. The dipole moment of the X-ray clusters does not coincide with that of the microwave background dipole. The two-point correlation function of the X-ray clusters is unity on a scale of about 2000 km/s.

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