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Astron. Astrophys. 331, 1108-1112 (1998)

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4. Conclusion

We showed that caustics complement the information provided by the Poincaré surface of section. If we consider both methods, we can determine the values of p and q for the [FORMULA] resonance for every orbit. So we conclude that the method can help us to understand a bit more about the complexity of non-linear Hamiltonian systems.

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© European Southern Observatory (ESO) 1998

Online publication: March 3, 1998
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