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Computer Simulations of Galaxy Clustering

Published online by Cambridge University Press:  14 August 2015

Sverre J. Aarseth
Sverre J. Aarseth*
Affiliation:
Institute of Astronomy University of Cambridge, England

Extract

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The aim of the present work (performed in collaboration with J.R. Gott and E.L. Turner) is to account for the observed distribution of galaxies in terms of the gravitational instability picture. Specifically we assume that all the matter is contained in galaxies. the evolution of such a system can then be studied by N-body simulations once the initial conditions are specified. Our approach is essentially experimental; a variety of models are computed and the results are compared with observations.

Type
II. Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 189 - 196
Copyright
Copyright © Reidel 1978 

References

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