On the Stability of the Triangular Libration Points for the Photogravitational Circular Restricted Problem of Three Bodies Under the Resonances of the Third and the Fourth Order

Details On the Stability of the Triangular Libration Points for the Photogravitational Circular Restricted Problem of Three Bodies Under the Resonances of the Third and the Fourth Order On the Stability of the Triangular Libration Points for the Photogravitational Circular Restricted Problem of Three Bodies Under the Resonances of the Third and the Fourth Order

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cemec..41..161k&link_type=abstract

Celestial Mechanics, Volume 41, Issue 1-4, pp. 161-173

Physics

2

Scientific paper

The authors investigate the stability of the triangular libration points
when both the attracting bodies are radiating under the resonance
conditions ω1 = 2ω2 and
3ω2.

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