Hostname: page-component-745bb68f8f-hvd4g Total loading time: 0 Render date: 2025-01-12T18:55:20.238Z Has data issue: false hasContentIssue false
  • English
  • Français

Galaxy formation modeling

Published online by Cambridge University Press:  06 October 2004

Andrew J. Benson
Andrew J. Benson
Affiliation:
Department of Physics, University of Oxford, Keble Road, Oxford, OX1 3RH, U.K. email: abenson@astro.ox.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Ab-initio modeling of galaxy formation is becoming ever more detailed and is including ever more physical processes in a bid to describe the process of galaxy formation more realistically. We will describe some recent advances and applications of the semi-analytic model of galaxy formation, GALFORM. In particular, we will describe a preliminary study of the effects of environment on galaxy morphology in a $z=0.4$ cluster.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 527 - 533
Copyright
© 2004 International Astronomical Union