Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-27T10:05:26.485Z Has data issue: false hasContentIssue false
  • English
  • Français

A Magnetohydrodynamic Model of Galaxy Formation

Published online by Cambridge University Press:  12 April 2016

J. P. Sleath  and
A. H. Nelson
J. P. Sleath
Affiliation:
Department of Physics and Astronomy, University of Wales College of Cardiff, P.O. Box 913, Cardiff, CF2 3YB, U.K.
A. H. Nelson
Affiliation:
Department of Physics and Astronomy, University of Wales College of Cardiff, P.O. Box 913, Cardiff, CF2 3YB, U.K.

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.

We present a full 3D model of galaxy formation, incorporating for the first time magnetohydrodynamical effects. By this means we hope to simulate the creation of active galactic nuclei, including jets. Preliminary results are encouraging.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 797 - 798
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Beck, R., & Hoernes, P. 1996, Nature, 379, 47 Google Scholar
Fitt, A.J., & Alexander, P. 1993, MNRAS, 261, 445 Google Scholar
Hernquist, L., & Katz, N. 1989, ApJS, 70, 419 Google Scholar
Kronberg, P.P., Perry, J.J., & Zukowski, E.L.H. 1992, ApJ, 387, 528 Google Scholar
Ratra, B. 1992, ApJ, 391, L1 CrossRefGoogle Scholar