Secular dynamics of the three-body problem: application to the "úpsilon" Andromedae planetary system (2004)
- Authors:
- Autor USP: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- Subjects: MECÂNICA CELESTE; PLANETAS
- Language: Inglês
- Imprenta:
- Source:
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ABNT
MICHTCHENKO, Tatiana Alexandrovna e MALHOTRA, Ripudaman. Secular dynamics of the three-body problem: application to the "úpsilon" Andromedae planetary system. Icarus, v. 168, p. 237-248, 2004Tradução . . Acesso em: 23 abr. 2024. -
APA
Michtchenko, T. A., & Malhotra, R. (2004). Secular dynamics of the three-body problem: application to the "úpsilon" Andromedae planetary system. Icarus, 168, 237-248. -
NLM
Michtchenko TA, Malhotra R. Secular dynamics of the three-body problem: application to the "úpsilon" Andromedae planetary system. Icarus. 2004 ;168 237-248.[citado 2024 abr. 23 ] -
Vancouver
Michtchenko TA, Malhotra R. Secular dynamics of the three-body problem: application to the "úpsilon" Andromedae planetary system. Icarus. 2004 ;168 237-248.[citado 2024 abr. 23 ] - On the V-type asteroids outside the Vesta family: is(21238)1995 WV7 a former member of the Eunomia family?
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- On the current distribution of the main belt objects:: constraints for the evolutionary models
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- A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances
- Discovery of a basaltic asteroid in the outer main belt
- The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis
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