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Stability of S-type orbits in binaries

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Publication:1610330
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DOI10.1023/A:1014586308539zbMath1192.70013WikidataQ108439667 ScholiaQ108439667MaRDI QIDQ1610330

E. Pilat-Lohinger, Rudolf Dvorak

Publication date: 19 August 2002

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)


zbMATH Keywords

fast Lyapunov indicatorsdouble starsS-type motion


Mathematics Subject Classification ID

Stability for nonlinear problems in mechanics (70K20) Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)


Related Items (5)

Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories ⋮ The rectilinear three-body problem as a basis for studying highly eccentric systems ⋮ Massive evaluation and analysis of Poincaré recurrences on grids of initial data: a tool to map chaotic diffusion ⋮ Stability criteria for hierarchical triple systems ⋮ On the Stability of Extra-Solar Planetary Systems







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