Hostname: page-component-848d4c4894-x5gtn Total loading time: 0 Render date: 2024-05-17T18:39:35.319Z Has data issue: false hasContentIssue false
  • English
  • Français

Two–Integral Models with Almost Circular Orbits

Published online by Cambridge University Press:  07 August 2017

P. Batsleer  and
H. Dejonghe
P. Batsleer
Affiliation:
Sterrenkundig Observatorium, Gent, Belgium
H. Dejonghe
Affiliation:
Sterrenkundig Observatorium, Gent, Belgium

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 global dynamical models for bulge–disk systems. The phase–space structure is examined by means of two integral models. The models indicate that in the formation merger argument for ellipticals one cannot always assume that the maximum phase–space density occurs in the center of the system.

Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 359 - 360
Copyright
Copyright © Kluwer 1993 

References

Dejonghe, H., 1989, ApJ, 343, 113.CrossRefGoogle Scholar
Gilmore, G., King, I., van der Kruit, P. in The Milky as a Galaxy, Geneva Observatory.Google Scholar
Kruit, P.C. van der and Searle, L., 1982, AA, 110, 61.Google Scholar