Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-28T01:56:53.511Z Has data issue: false hasContentIssue false
  • English
  • Français

Planetary Nebulae in elliptical galaxies: Dynamical models for Centaurus A

Published online by Cambridge University Press:  25 May 2016

Anne Mathieu  and
Herwig Dejonghe
Anne Mathieu
Affiliation:
Sterrenkundig Observatorium, University of Ghent, Belgium
Herwig Dejonghe
Affiliation:
Sterrenkundig Observatorium, University of Ghent, Belgium

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 use planetary nebulae major- and minor-axis kinematics (Hui et al. 1995) of the dust-lane elliptical galaxy NGC 5128 (Centaurus A) to build triaxial dynamical models.

Type
VIII. Planetary Nebulae in Extragalactic Systems
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 472
Copyright
Copyright © Kluwer 1997 

References

Hui, X., Ford, H. C., Freeman, K. C., Dopita, M. A., 1995, Astrophys. Journ., 449, 592.Google Scholar
Mathieu, A., Dejonghe, H., Hui, X., 1996a, Astron. Astrophys., 309, 30.Google Scholar
Mathieu, A., Dejonghe, H., 1996b, Astron. Astrophys., 314, 25.Google Scholar