Sathyaprakash, Bangalore Suryanarayana ![]() |
Official URL: http://dx.doi.org/10.1086/311689
Abstract
We explore the shapes of clusters and superclusters in the IRAS 1.2 Jy redshift survey with three reconstructions spanning the range β=0.1, 0.5, and 1.0, where β=Ω0.6/b; b is the bias factor, and Ω is the present value of the dimensionless matter density. Comparing our results with Gaussian randomized reconstructions of the IRAS catalog, we find structures having both planar and filamentary properties. For β=0.5 and 1.0, the largest structures in the survey have a distinct tendency to be filament-like, in general agreement with the results of N-body simulations.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | cosmology: theory—galaxies: clusters: general—infrared: galaxies— large-scale structure of universe—methods: analytical—methods: numerical |
Publisher: | IOP Publishing |
ISSN: | 0004-637X |
Last Modified: | 24 Oct 2022 10:49 |
URI: | https://orca.cardiff.ac.uk/id/eprint/45971 |
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