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The Construction of Stäckel Potentials for Galactic Dynamical Modelling

Published online by Cambridge University Press:  07 August 2017

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

Abstract

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We present a set of axisymmetric Stäckel potentials which can be used for Galactic dynamical modelling. Each of them has a halo–disk structure with a flat rotation curve.

Type
Contributed Papers
Copyright
Copyright © Kluwer 1993 

References

Bahcall, J.N., Schmidt, M., and Soneira, R. M., 1982, ApJ L23, 258.Google Scholar
Dejonghe, H. and de Zeeuw, P.T. 1988a, ApJ, 333, 90.Google Scholar
Dejonghe, H. and de Zeeuw, P.T. 1988b, ApJ, 329, 720.CrossRefGoogle Scholar
Gilmore, G., King, I., Van der Kruit, P. 1989, The Milky way as a Galaxy, ed. Buser, R, and King, I. (Geneva Observatory).Google Scholar
Kuzmin, G.G., and Kutuzov, S.A. 1962, Bull. Abastumani Ap. Obs., 27, 82.Google Scholar
Rubin, V.C., Burstein, D. Ford, W.K., and Thonnard, N. 1985, ApJ, 289, 81.Google Scholar