Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system (2006)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- Subjects: MECÂNICA CELESTE; PLANETAS
- Language: Inglês
- Imprenta:
- Source:
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ABNT
MICHTCHENKO, Tatiana Alexandrovna e FERRAZ-MELLO, Sylvio e BEAUGÉ, C. Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system. Icarus, v. 181, n. 2, p. 555-571, 2006Tradução . . Acesso em: 29 dez. 2025. -
APA
Michtchenko, T. A., Ferraz-Mello, S., & Beaugé, C. (2006). Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system. Icarus, 181( 2), 555-571. -
NLM
Michtchenko TA, Ferraz-Mello S, Beaugé C. Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system. Icarus. 2006 ; 181( 2): 555-571.[citado 2025 dez. 29 ] -
Vancouver
Michtchenko TA, Ferraz-Mello S, Beaugé C. Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system. Icarus. 2006 ; 181( 2): 555-571.[citado 2025 dez. 29 ] - Extra-solar planetary systems
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- On the similarities and differences between 3/2 and 2/1 asteroidal resonances
- Tidal evolution of a close-in planet with a more massive outer companion
- Dynamics of two planets in co-orbital motion
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