Model Predictions for Clustering and Morphologies at HDF depths

Details Model Predictions for Clustering and Morphologies at HDF depths Model Predictions for Clustering and Morphologies at HDF depths

1998-01-05

arxiv.org/abs/astro-ph/9801025v1

Astronomy and Astrophysics

Astrophysics

invited review given at the STScI May Symposium "The Hubble Deep Field" 13 pages, 7 figures included

Scientific paper

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.

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