The stability of binary star systems during encounters with a third star

DOI10.1093/MNRAS/210.4.915zbMath0538.70016OpenAlexW2006110155MaRDI QIDQ3325098

J. R. Donnison

Publication date: 1984

Published in: Monthly Notices of the Royal Astronomical Society (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1093/mnras/210.4.915

zbMATH Keywords

collisiondisruptionbinary systemstable motionthree-body zero velocity surfaces

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15) Collision of rigid or pseudo-rigid bodies (70F35)

Related Items (3)

Stability criteria for hierarchical triple systems ⋮ Systematic simulations of FFP scattering by a star-planet pair ⋮ Limits on the orbits of possible eccentric and inclined moons of extrasolar planets orbiting single stars

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