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

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

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26at...24..311b&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 24, Issue 4, p.311-316

Astronomy and Astrophysics

Astronomy

3

Dynamics, Non-Stationary Systems, Particular Solutions

Scientific paper

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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