The 2/1 and 3/2 Resonant Asteroid Motion: A Symplectic Mapping Approach
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Publisher
Springer Netherlands
Link
http://link.springer.com/content/pdf/10.1007/978-94-017-2414-2_9
Reference17 articles.
1. Ferraz-Mello, S.: 1997, ‘A symplectic mapping approach to the study of the stochasticity of asteroidal resonances’, Celest. Mech. and Dyn. Astr. 65, 421 – 437.
2. Ferraz-Mello, S., Michtchenko, T. A., Nesvorny, D., Roig, F. and Simula, A.: 1998, ‘The depletion of the Hecuba Gap vs. the long-lasting Hilda group’, Planet. Space Sci. 46, 1425 – 1432.
3. Hadjidemetriou, J. D.: 1993, ‘Asteroid motion near the 3:1 resonance’, Celest. Mech. and Dyn. Aste. 56, 563–599.
4. Hadjidemetriou, J. D. and Lemaitre, A.: 1997, ‘Asteroid Motion near the 2:1 Resonance: A Symplectic Mapping Approach’, in: R. Dvorak and J. Henrard (eds), The Dynamical Behaviour of our Planetary System, Kluwer Acad. Publ. pp. 277 – 290.
5. Hadjidemetriou, J. D.: 1999, ‘A symplectic mapping model as a tool to understand the dynamics of the 2/1 resonant asteroid motion’, Celest. Mech. and Dyn. Aste. 73, 65–76.
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