Model Predictions for Clustering and Morphologies at HDF depths
Astrophysics
2007-05-23 v1
Abstract
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.
Cite
@article{arxiv.astro-ph/9801025,
title = {Model Predictions for Clustering and Morphologies at HDF depths},
author = {Matthias Steinmetz},
journal= {arXiv preprint arXiv:astro-ph/9801025},
year = {2007}
}
Comments
invited review given at the STScI May Symposium "The Hubble Deep Field" 13 pages, 7 figures included