Hostname: page-component-7479d7b7d-jwnkl Total loading time: 0 Render date: 2024-07-09T01:28:27.862Z Has data issue: false hasContentIssue false
  • English
  • Français

The Formation of Galaxy Disks and Bulges

Published online by Cambridge University Press:  25 May 2016

P.R. Williams  and
A.H. Nelson
P.R. Williams
Affiliation:
Department of Physics and Astronomy, University of Wales, College Cardiff, PO Box 913, Cardiff, CF2 3YB
A.H. Nelson
Affiliation:
Department of Physics and Astronomy, University of Wales, College Cardiff, PO Box 913, Cardiff, CF2 3YB

Extract

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.

Using a TREESPH code modified to run on a parallel computer and a new algorithm for modeling star formation, we have investigated the formation of disk galaxies from idealized cosmological perturbations.

Type
Deep Fields & Evolution
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 490
Copyright
Copyright © Kluwer 1999 

References

Steinmetz, M., & Müller, E. 1995, MNRAS, 276, 549 Google Scholar