Hostname: page-component-f554764f5-fr72s Total loading time: 0 Render date: 2025-04-09T19:59:10.506Z Has data issue: false hasContentIssue false
  • English
  • Français

Typical Motions in Multiple Systems

Published online by Cambridge University Press:  12 April 2016

Joanna Anosova
Joanna Anosova*
Affiliation:
Astronomical Observatory Leningrad University, USSR

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In very old times, people counted – one, two, many. I want to show you now that they were right.

Let’s consider the motions of isolated bodies:

  1. 1. N = 1 - simple motion;

  2. 2. N = 2 - Keplerian orbits;

  3. 3. N = 3 - this is the difficult problem. In general, this problem can be studied only by computer simulations.

Type
VIII. Classical Theory of Multiplets
Information
International Astronomical Union Colloquium , Volume 124: Paired and Interacting Galaxies , 1990 , pp. 629 - 631
Copyright
Copyright © NASA 1990

References

Agekian, T. A., and Anosova, J. P. 1967, Sov. Astron. Journ., 44, 6, p. 1261–1273.Google Scholar
Anosova, J. P. 1986, Astrophysics and Space Science, 124, 2, p. 217–241.CrossRefGoogle Scholar
Anosova, J. P. 1989a, Comments on Astrophysics, 1414, 1, p. 17–36.Google Scholar
Anosova, J. P. 1989b, Comments on Astrophysics, 14, 1, p. 37–60.Google Scholar