The Evolution of Galaxy Clustering in Hierarchical Models

Preprint

13 October 1999

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9910233

Abstract

The main ingredients of recent semi-analytic models of galaxy formation are summarised. We present predictions for the galaxy clustering properties of a well specified LCDM model whose parameters are constrained by observed local galaxy properties. We present preliminary predictions for evolution of clustering that can be probed with deep pencil beam surveys.

Keywords

HIERARCHICAL MODELS
GALAXY CLUSTERING
MAIN INGREDIENTS
ANALYTIC MODELS
WELL SPECIFIED
PROPERTIES
EVOLUTION
SURVEYS

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Version 1, 1999-10-13, ArXiv

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