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Inversions for axisymmetric galactic disks
Authors:N Hiotelis  P A Patsis
Institution:(1) Department of Mathematics, Hellenic Air Force Academy, Dekeleia, Attica, Greece;(2) Department of Astronomy, University of Athens, Greece;(3) E.S.O., Garching-bei-München, Germany
Abstract:We use two models for the distribution function to solve an inverse problem for axisymmetric disks. These systems may be considered - under certain assumptions - as galactic disks. In some cases the solutions of the resulting integral equations are simple, which allows the determination of the kinematic properties of self-consistent models for these systems. These properties for then = 1 Toomre disk are presented in this study.
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