Theoretically Observable Signatures of a Stable Three-Body Figure-8 Orbit

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Scientific paper

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Scientific paper

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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