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Results:
1-8
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Results: 8
Authors:
Bottke, WF
Vokrouhlicky, D
Broz, M
Nesvorny, D
Morbidelli, A
Citation: Wf. Bottke et al., Dynamical spreading of asteroid families by the Yarkovsky effect, SCIENCE, 294(5547), 2001, pp. 1693-1696
Mean motion resonances in the transneptunian region part II: The 1 : 2, 3 : 4, and weaker resonances
Authors:
Nesvorny, D
Roig, F
Citation: D. Nesvorny et F. Roig, Mean motion resonances in the transneptunian region part II: The 1 : 2, 3 : 4, and weaker resonances, ICARUS, 150(1), 2001, pp. 104-123
Authors:
Nesvorny, D
Roig, F
Citation: D. Nesvorny et F. Roig, Mean motion resonances in the trans-Neptunian region I. The 2 : 3 resonance with Neptune, ICARUS, 148(1), 2000, pp. 282-300
Authors:
Nesvorny, D
Roig, F
Ferraz-Mello, S
Citation: D. Nesvorny et al., Close approaches of trans-Neptunian objects to Pluto have left observable signatures on their orbital distribution, ASTRONOM J, 119(2), 2000, pp. 953-969
Authors:
Morbidelli, A
Nesvorny, D
Citation: A. Morbidelli et D. Nesvorny, Numerous weak resonances drive asteroids toward terrestrial planets orbits, ICARUS, 139(2), 1999, pp. 295-308
Authors:
Nesvorny, D
Morbidelli, A
Citation: D. Nesvorny et A. Morbidelli, An analytic model of three-body mean motion resonances, CEL MEC DYN, 71(4), 1998, pp. 243-271
Authors:
Ferraz-Mello, S
Michtchenko, TA
Nesvorny, D
Roig, F
Simula, A
Citation: S. Ferraz-mello et al., The depletion of the Hecuba gap vs the long-lasting Hilda group, PLANET SPAC, 46(11-12), 1998, pp. 1425-1432
Authors:
Nesvorny, D
Morbidelli, A
Citation: D. Nesvorny et A. Morbidelli, Three-body mean motion resonances and the chaotic structure of the asteroid belt, ASTRONOM J, 116(6), 1998, pp. 3029-3037
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