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Hierarchical and Non-Hierarchical Triples

Published online by Cambridge University Press:  25 May 2016

J. Anosova ,
L. Kiseleva ,
P. Eggleton  and
V. Orlov
J. Anosova
Affiliation:
National Astronomical Observatory, Tokyo 181, Japan
L. Kiseleva
Affiliation:
Institute of Astronomy, Cambridge CB3 0HA, UK
P. Eggleton
Affiliation:
Institute of Astronomy, Cambridge CB3 0HA, UK
V. Orlov
Affiliation:
Astronomical Institute, St. Peterburgh University, St. Petersburg 198904, Russia

Extract

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Triple stars and galaxies are referred to as having hierarchical or non-hierarchical structure. Thus, the dynamically stable and unstable triple systems are usually distinguished observationally by the ratio of the larger and smaller angular separation. However, (i) projection effects may hide the true configuration; and (ii) apparent hierarchical forms may occur in both types (Anosova 1986).

Type
Chapter 6: How are we to Understand the Large Scale Structure of the ISM?
Information
Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 529 - 530
Copyright
Copyright © Kluwer 1996 

References

Anosova, J. Astrophys. Space Sci., 1986, 124, 217.Google Scholar
Anosova, J., Orlov, V., Cel. Mech. and Dyn. Astr., 1994, 59, 327.Google Scholar
Kiseleva, L., Eggleton, P. Anosova, J. 1994. MNRAS, 267, 161.CrossRefGoogle Scholar
Kiseleva, L., Eggleton, P., Orlov, V. 1994. MNRAS, in press Google Scholar