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D. Terry, T. E. Nordgren, A. J. DeWeerd (U. of Redlands)
The figure-eight has been found to be a stable, periodic solution to the equal mass three body problem. The three bodies traverse the path of the eight with a phase shift from each other of one-third of a period. We use a numerical model of this solution in order to identify observable stellar signatures of such an orbit should one really exist.
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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.