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Flattened γ models for galaxies

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Using the equipotential method we introduce a class of flattened γ models for galaxies and study the properties of their potential–density pairs and two-integral distribution functions.

Keywords: Celestial mechanics; Kinematics; Stellar dynamics; Structure of galaxies

Document Type: Research Article


Affiliations: 1: Department of Mathematics, Zhongzhan University, Guangzhou, 510275, PR China 2: Department of Space Technologies and Applied Astrodynamics, St Petersburg State University, Universitetskij Prospekt 35, Staryj Peterhof, St Petersburg, 198504, Russia

Publication date: 2006-04-01

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