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Local density maxima - Progenitors of structure

Hoffman, Y., Shaham, J.·1985·The Astrophysical Journal

Abstract

Beginning with a short review of the observational data and of some previous theoretical ideas and numerical simulations, the question is addressed of how the large-scale structure that emerges around local density maxima depends on the nature of the primordial density perturbations field. The density contrast profile around local maxima is given, to a good approximation, by the primordial two-point correlation function. The mean number density of objects of a given core mass is calculated as a function of the primordial power spectrum, p(k). In an open universe, rich clusters should have halos steeper than galactic haloes. The observed structure is found to be consistent with omega-sub-zero less than 1.0 and n = -1.

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Metadata

Authors
Hoffman, Y., & Shaham, J.
Venue
The Astrophysical Journal
Published
1985-10
Volume
297
Pages
16
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1983113556
Cited by
203
References
0
FWCI
3.86
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Local density maxima - Progenitors of structure. https://app.cochat.ai/papers/10.1086/163498
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Hoffman, Y., & Shaham, J. (1985). Local density maxima - Progenitors of structure. The Astrophysical Journal. https://doi.org/10.1086/163498

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.