Abstract
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.
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References
Binggeli, B. 1982, Astron. Astrophys. (in press).
Einasto, J., Jôeveer, M., Saar, E. 1980, M.N.R.A.S., 193, 353.
Einasto, J., Klypin, A., Saar, E., Shandarin, S. 1982 (in preparation).
Jôeveer, M., Einasto, J., and Tago, E. 1978, M.N.R.A.S., 185, 357.
Peebles, P.J.E. 1980, The Large-Scale Structure of the Universe, Princeton University Press.
Shandarin, S.F. 1982, Pis’ma v AZh (in press).
Soneira, R.M., and Peebles, P.J.E. 1978, Astron. J., 83, 845.
Zeldovich, Ya.B., Einasto, J., and Shandarin, S.F. 1982 (preprint).
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© 1983 IAU
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Einasto, J., Klypin, A., Shandarin, S. (1983). Structure of Neighboring Superclusters: A Quantitative Analysis. In: Abell, G.O., Chincarini, G. (eds) Early Evolution of the Universe and its Present Structure. International Astronomical Union / Union Astronomique Internationale, vol 104. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7220-9_65
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DOI: https://doi.org/10.1007/978-94-009-7220-9_65
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-1662-0
Online ISBN: 978-94-009-7220-9
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