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Two–Integral Models with Almost Circular Orbits
Published online by Cambridge University Press: 07 August 2017
Abstract
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We present global dynamical models for bulge–disk systems. The phase–space structure is examined by means of two integral models. The models indicate that in the formation merger argument for ellipticals one cannot always assume that the maximum phase–space density occurs in the center of the system.
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- Copyright © Kluwer 1993
References
Gilmore, G., King, I., van der Kruit, P. in The Milky as a Galaxy, Geneva Observatory.Google Scholar
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