The Stroboscopic Method Applied to the Stellar Three-Body Problem: The Keplerian Outer Orbit Approximation

Details The Stroboscopic Method Applied to the Stellar Three-Body Problem: The Keplerian Outer Orbit Approximation The Stroboscopic Method Applied to the Stellar Three-Body Problem: The Keplerian Outer Orbit Approximation

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aj....110..875l&link_type=abstract

Astronomical Journal v.110, p.875

Astronomy and Astrophysics

Astronomy

1

Celestial Mechanics

Scientific paper

This article discusses the stellar three-body problem using an approximation in which the outer orbit is assumed to be Keplerian. The equations of motion are integrated by the stroboscopic method, i.e., basically at successive periods of a rapidly changing variable (the eccentric anomaly of the inner orbit). The theory is applied to the triple-star system ξ Ursae Majoris.

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