Model for the study of very-high-eccentricity asteroidal motion the 3: 1 resonance (1991)
- Authors:
- USP affiliated authors: MELLO, SYLVIO FERRAZ DE - IAG ; KLAFKE, JULIO CESAR - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Inglês
- Imprenta:
- Publisher: Plenum Press
- Publisher place: New York
- Date published: 1991
- Source:
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ABNT
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: 13 fev. 2026. -
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 2026 fev. 13 ] -
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 2026 fev. 13 ] - Sobre algumas características de asteróides em ressonância 3 / 1 com júpiter segundo método de delaunay estendido
- Chaotic transitions in resonant asteroidal dynamics
- Chaotic transitions in resonant asteroidal dynamics
- Estrutura de alta excentricidade da ressonância 3: 1
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- Modelo plano para o estudo das ressonâncias asteroidais de alta excentricidade
- Very-high- eccentricity librations at some higher order resonances
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