Abstract
Many elliptical galaxies may be slowly rotating, moderately triaxial systems. Their dynamics are probably characteristic of a 1:1:1-resonance between the frequencies of oscillation along the three principal axes.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Similar content being viewed by others
References
van Albada, T.S., Kotanyi, C.G. and Schwarzschild, M.: 1982, M.N.R.A.S., 198, 303.
Heisler, J., Merritt, D.R. and Schwarzschild, M.: 1982, Astrophys. J., 258, 490.
Magnenat, P.: 1982, Astron. Astrophs. 108, 89.
Martinet, L.: 1982, Proceedings of the CECAM Workshop on Structure, Formation and Evolution of Galaxies, held in Paris, August 1981 (eds. J. Audouze and C.A. Norman).
Schwarzschild, M.: 1979, Astrophys. J. 232, 236.
de Zeeuw, P.T.: 1982, Proceedings of the CECAM Workshop on Structure, Formation and Evolution of Galaxies, held in Paris, August 1981 (eds. J. Audouze and C.A. Norman).
de Zeeuw, P.T. and Merritt, D.R.: 1982, submitted to Astrophys. J.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1983 IAU
About this chapter
Cite this chapter
Martinet, L., de Zeeuw, T. (1983). Three-Dimensional Orbits in Triaxial Galaxies. In: Athanassoula, E. (eds) Internal Kinematics and Dynamics of Galaxies. International Astronomical Union/Union Astronomique Internationale, vol 100. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7075-5_78
Download citation
DOI: https://doi.org/10.1007/978-94-009-7075-5_78
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-1547-0
Online ISBN: 978-94-009-7075-5
eBook Packages: Springer Book Archive