CAOSP abstracts, Volume: 33, No.: 3, year: 2003


Abstract: The analytical theory of the general three-body problem to real triple stellar systems is applied. On the stellar systems ξ UMa, ζ Aqu, and AS Cam it is shown how this theory can be used for the investigation of the dynamical evolution of triple stellar systems. It is possible to establish the moment of the close approach of the inner pair, and to define the secular and long-periodic perturbations in the motions of the periastrons and nodes.

Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.




Back to:
CAOSP Vol. 33 No. 3 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page

Valid HTML 4.01! Valid CSS!

Last update: November 10, 2003