Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-30T00:41:12.066Z Has data issue: false hasContentIssue false
  • English
  • Français

Structure of Neighboring Superclusters: A Quantitative Analysis

Published online by Cambridge University Press:  04 August 2017

J. Einasto ,
A. Klypin  and
S. Shandarin
J. Einasto
Affiliation:
Tartu Astrophysical Observatory, Institute of Applied Mathematics, Moscow
A. Klypin
Affiliation:
Tartu Astrophysical Observatory, Institute of Applied Mathematics, Moscow
S. Shandarin
Affiliation:
Tartu Astrophysical Observatory, Institute of Applied Mathematics, Moscow

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

So far the galaxy correlation analysis was the only quantitative method used to describe the distribution of galaxies in space. Here we consider other numerical methods to treat impersonally various aspects of the galaxy distribution.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 265 - 271
Copyright
Copyright © Reidel 1983 

References

Binggeli, B. 1982, Astron. Astrophys. (in press).Google Scholar
Einasto, J., Jôeveer, M., Saar, E. 1980, M.N.R.A.S., 193, 353.CrossRefGoogle Scholar
Einasto, J., Klypin, A., Saar, E., Shandarin, S. 1982 (in preparation).Google Scholar
Jôeveer, M., Einasto, J., and Tago, E. 1978, M.N.R.A.S., 185, 357.CrossRefGoogle Scholar
Peebles, P.J.E. 1980, The Large-Scale Structure of the Universe, Princeton University Press.Google Scholar
Shandarin, S.F. 1982, Pis'ma v AZh (in press).Google Scholar
Soneira, R.M., and Peebles, P.J.E. 1978, Astron. J., 83, 845.CrossRefGoogle Scholar
Zeldovich, Ya.B., Einasto, J., and Shandarin, S.F. 1982 (preprint).Google Scholar