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On the dynamics of non-stationary binary stellar systems with non-isotropic mass flow

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The motion of a test body in the external gravitational field of binary stellar systems with some slowly varying physical parameters of the radiating components is considered on the basis of the restricted non-stationary photogravitational three- and two-body problems with non-isotropic mass flow. The family of polar and coplanar solutions are obtained. These solutions make it possible to give a dynamic and structural interpretation of binary young evolving stars and galaxies.
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Keywords: Dynamics; Non-stationary systems; Particular solutions

Document Type: Research Article

Affiliations: 1: Fesenkov Astrophysical Institute, 480020, Almaty, Kazakhstan 2: Kokshetau University, Kokshetau, Kazakhstan 3: Kazakh National Agrarian University, Almaty, Kazakhstan

Publication date: 2005-08-01

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