Model Predictions for Clustering and Morphologies at HDF depths

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dc.creatorSteinmetz, Matthias
dc.date1998-01-05
dc.date.accessioned2026-07-07T02:25:43Z
dc.date.available2026-07-07T02:25:43Z
dc.descriptionThe 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.
dc.descriptioninvited review given at the STScI May Symposium "The Hubble Deep Field" 13 pages, 7 figures included
dc.identifierhttps://arxiv.org/abs/astro-ph/9801025
dc.identifierhttp://arxiv.org/abs/astro-ph/9801025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11986
dc.subjectAstrophysics
dc.titleModel Predictions for Clustering and Morphologies at HDF depths
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