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Analytical models for rotating and flattened perturbations in bulges

Published online by Cambridge University Press:  07 August 2017

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

Abstract

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A power series approach for solving the linearized transport equation for perturbations in the central part of flat disks is presented. The application of this method is in principle independent of the mathematical complexity of the unperturbed distribution. As an illustration, this method was used to solve the transport equation in the case of Kalnajs' Omega models.

Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 381 - 382
Copyright
Copyright © Kluwer 1993 

References

Dejonghe, H., 1984, (unpublished)Google Scholar
Hunter, C., 1963, MNRAS, 126, 299.Google Scholar
Kalnajs, A., 1972, Astrophys. J., 175, 63 Google Scholar