The Evolution of Galaxy Clustering in Hierarchical Models

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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.
To appear in the proceedings of the Marseille IGRAP99 conference "Clustering at High Redshift"

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/14999

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9910233
 http://arxiv.org/abs/astro-ph/9910233

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arXiv