Abstract
The use of precise numerical integrations and Fourier analysis techniques allowed us an investigation of the regular motions of asteroids near the 3:2 resonance with Jupiter (Hildas). The results are shown and compared to similar results previously obtained with analytical models.
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© 1993 Springer Science+Business Media Dordrecht
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Michtchenko, T., Ferraz-Mello, S. (1993). The High-Eccentricity Libration of the Hildas II. Synthetic-Theory Approach. In: Dvorak, R., Henrard, J. (eds) Qualitative and Quantitative Behaviour of Planetary Systems. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2030-2_11
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DOI: https://doi.org/10.1007/978-94-011-2030-2_11
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