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The large-scale distribution of galaxiesThe spatial distribution of galaxies in the universe is characterized on the basis of the six completed strips of the Harvard-Smithsonian Center for Astrophysics redshift-survey extension. The design of the survey is briefly reviewed, and the results are presented graphically. Vast low-density voids similar to the void in Bootes are found, almost completely surrounded by thin sheets of galaxies. Also discussed are the implications of the results for the survey sampling problem, the two-point correlation function of the galaxy distribution, the possibility of detecting large-scale coherent flows, theoretical models of large-scale structure, and the identification of groups and clusters of galaxies.
Document ID
19900057028
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Geller, Margaret J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Subject Category
Astrophysics
Meeting Information
Meeting: ESO-CERN Symposium on Astronomy, Cosmology and Fundamental Physics
Location: Bologna
Country: Italy
Start Date: May 16, 1988
End Date: May 20, 1988
Sponsors: Universita di Bologna, Istituto Nazionale di Fisica Nucleare, CNR
Accession Number
90A44083
Funding Number(s)
CONTRACT_GRANT: NAGW-201
Distribution Limits
Public
Copyright
Other

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