A deep Abell cluster redshift survey

Details A deep Abell cluster redshift survey A deep Abell cluster redshift survey

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...365...66h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 365, Dec. 10, 1990, p. 66-85. Research supported by the Smithsonian Institu

Astronomy and Astrophysics

Astronomy

99

Galactic Clusters, Red Shift, Sky Surveys (Astronomy), Interacting Galaxies, Monte Carlo Method, Spatial Distribution

Scientific paper

Redshifts have been measured for a complete sample of 145 Abell clusters of galaxies of median redshift 0.16 covering a 561 sq deg region at high Galactic latitude. Clustering on scales greater than about 70/h Mpc cannot be detected. A large void of diameter about 20,000 km/s seen in maps of the cluster distribution is consistent with smaller scale behavior of the correlation function of the survey. Large-scale peculiar motions are about 1000 km/s or less, a limit inconsistent with the claimed detection by Bahcall et al. (1986) of peculiar motions of about 2000 km/s.

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