Annotation
The work is devoted to the application of the stellar three-body problem to the system ξU.Ma. We determine the secular variations of longitudes of the nodes and periastrons of the components of the system, and made a comparison with the results of Brownrs theory.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
A.A. Оrlоv, N.A. Sоlоvауa
Sternberg Astronomical Institute, Moscow State University Universitetsky pr., 13, Moscow 119234, Russia
Sternberg Astronomical Institute, Moscow State University Universitetsky pr., 13, Moscow 119234, Russia
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