The origin or large-scale periodicity

Details The origin or large-scale periodicity The origin or large-scale periodicity

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..222..276b&link_type=abstract

After the first three minutes. AIP Conference Proceedings, Volume 222, pp. 276-282 (1991).

Physics

Observational Cosmology

Scientific paper

The apparent ~130 h-1 Mpc periodic distribution of galaxies recently observed in pencil-beam surveys is shown to originate in known large-scale superclusters. The superclusters, covering the high-latitude sky to z<=0.08, show the same peaks that appear in the pencil-beam survey, indicating that the galaxy peaks are drawn from these superclusters. Predictions for future pencil-beam surveys in different directions are given. The results suggest a network structure of large (~100 h-1 Mpc) supercluster surfaces surrounding low density regions.

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