Hill stability and distance curves for the general three-body problem
- 1 March 1982
- journal article
- Published by Springer Nature in Celestial Mechanics and Dynamical Astronomy
- Vol. 26 (3), 311-333
- https://doi.org/10.1007/bf01230725
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Stability of planetary orbits in binary systemsCelestial Mechanics and Dynamical Astronomy, 1980
- Stability of artificial and natural satellitesCelestial Mechanics and Dynamical Astronomy, 1978
- Analytical determination of the measure of stability of triple stellar systemsCelestial Mechanics and Dynamical Astronomy, 1977
- Stability of planetary systems with bifurcation theoryThe Astronomical Journal, 1977
- Zero velocity surfaces for the general planar three-body problemAstrophysics and Space Science, 1976
- The effects of integrals on the totality of solutions of dynamical systemsCelestial Mechanics and Dynamical Astronomy, 1976
- Hill regions for the general three-body problemCelestial Mechanics and Dynamical Astronomy, 1975
- Topology and mechanics. IIInventiones Mathematicae, 1970
- Mémoire sur le problème des trois corpsActa Mathematica, 1913
- Researches in the Lunar TheoryAmerican Journal of Mathematics, 1878