Model Predictions for Clustering and Morphologies at HDF depths

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The current status of numerical simulations of the formation of galaxies is reviewed. Success and failure of modeling galaxies at low and high redshift is demonstrated using a variety of examples, such as the Tully-Fisher relation, the appearance of high-redshift galaxies and the kinematics of damped Lya systems. The relationship between the clustering properties of high-z galaxies and the present generation of galaxies is emphasized.
invited review given at the STScI May Symposium "The Hubble Deep Field" 13 pages, 7 figures included

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/11986

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9801025
 http://arxiv.org/abs/astro-ph/9801025

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arXiv