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Paper: The Galactic Bulge Modelling
Volume: 316, Order and Chaos in Stellar and Planetary Systems
Page: 334
Authors: Raspopova, N.V.
Abstract: Mass distribution models for the Milky Way bulge are briefly discussed. We use the special case n = 4 of Kuzmin's family of Stäckel potentials for bulge modelling. Equidensity surfaces of the model are similar spheroids. After truncating exterior part a finite size model is obtained. Unbounded model is also considered as it has no density jump on the border. In order to get concrete model in both cases parameters should be estimated. Kutuzov's interval method is suggested for this purpose.
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