Stability of classical triplets and of their hierarchy

Details Stability of classical triplets and of their hierarchy Stability of classical triplets and of their hierarchy

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....58..145s&link_type=abstract

Astronomy and Astrophysics, vol. 58, no. 1-2, June 1977, p. 145-152. NSF-NATO-supported research.

Astronomy and Astrophysics

Astrophysics

81

Celestial Mechanics, Hierarchies, Orbital Elements, Stellar Mass, Stellar Systems, Systems Stability, Triple Stars, Two Body Problem, Eccentricity, Numerical Integration, Ternary Systems, Three Body Problem

Scientific paper

The effects of the participating stellar masses, semi-major axes and
eccentricities on the stability and expected permanency of triple stars
and of Evans-type hierarchies are investigated analytically. The results
are compared with Harrington's numerically obtained stability ranges and
with observed classical triplets.

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