Model for the study of very-high-eccentricity asteroidal motion the 3: 1 resonance (1991)
Source: Predictability, Stability and Chaos in N-Body Dynamical Systems. Unidade: IAG
Assunto: ASTRONOMIA
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FERRAZ-MELLO, Sylvio e KLAFKE, J C. Model for the study of very-high-eccentricity asteroidal motion the 3: 1 resonance. Predictability, Stability and Chaos in N-Body Dynamical Systems. Tradução . New York: Plenum Press, 1991. . . Acesso em: 09 ago. 2024.APA
Ferraz-Mello, S., & Klafke, J. C. (1991). Model for the study of very-high-eccentricity asteroidal motion the 3: 1 resonance. In Predictability, Stability and Chaos in N-Body Dynamical Systems. New York: Plenum Press.NLM
Ferraz-Mello S, Klafke JC. Model for the study of very-high-eccentricity asteroidal motion the 3: 1 resonance. In: Predictability, Stability and Chaos in N-Body Dynamical Systems. New York: Plenum Press; 1991. [citado 2024 ago. 09 ]Vancouver
Ferraz-Mello S, Klafke JC. Model for the study of very-high-eccentricity asteroidal motion the 3: 1 resonance. In: Predictability, Stability and Chaos in N-Body Dynamical Systems. New York: Plenum Press; 1991. [citado 2024 ago. 09 ]
