Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-25T21:47:25.026Z Has data issue: false hasContentIssue false
  • English
  • Français

The Wavy-Pattern of Stellar Rotation Curves in SBO Galaxies

Published online by Cambridge University Press:  12 April 2016

H. Wozniak  and
D. Pfenniger
H. Wozniak
Affiliation:
Observatoire de Marseille, F-13248 Marseille cedex 4, France
D. Pfenniger
Affiliation:
Geneva Observatory, CH-1290 Sauverny, Switzerland

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.

We discuss the “rotation” curves of SB0 galaxies with self-consistent models constructed with Schwarzschild’s method. Their distribution functions are compared with that of N-body simulations.

Type
Part VIII. Counterrotating Phenomena, Models, Synthesis of Results
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 445 - 448
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Bettoni, D. 1989, AJ, 97, 79 Google Scholar
Bettoni, D., Galletta, G., & Vallenari, A. 1988, A&A, 197, 69 Google Scholar
Galletta, G. 1987, ApJ, 318, 531 CrossRefGoogle Scholar
Pfenniger, D. 1984, A&A, 141, 171 Google Scholar
Pfenniger, D. & Friedli, D. 1991, A&A, 252, 75 Google Scholar
Schwarzschild, M. 1979, ApJ, 232, 236 Google Scholar
Sparke, L. & Sellwood, J.A. 1987, MNRAS, 225, 653 Google Scholar
Wozniak, H. & Pfenniger, D. 1996, A&A, in preparationGoogle Scholar