Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-06-24T03:51:23.986Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Spiral Patterns Generated in Galaxy Interactions - A Survey

Published online by Cambridge University Press:  03 August 2017

K. J. Donner ,
S. Engström  and
B. Sundelius
K. J. Donner
Affiliation:
Institute of Theoretical Physics Chalmers University of Technology S-412 96 Göteborg Sweden
S. Engström
Affiliation:
Institute of Theoretical Physics Chalmers University of Technology S-412 96 Göteborg Sweden
B. Sundelius
Affiliation:
Institute of Theoretical Physics Chalmers University of Technology S-412 96 Göteborg Sweden

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 numerical survey of interactions of galaxies. For the considered disc model there is an almost one dimensional sequence of forms in the time evolution of the perturbed (main) system.

Type
IV- Models of Spiral Structure
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 131
Copyright
Copyright © Kluwer 1991