Dynamics of two planets in the 2:1 and 3:2 mean motion resonances (2002)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- Assunto: SISTEMA SOLAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Bulletin of the American Astronomical Society
- ISSN: 0002-7537
- Volume/Número/Paginação/Ano: v. 34, n. 3, p. 892, res. 30.01, 2002
-
ABNT
CALLEGARI JR., N e MICHTCHENKO, Tatiana Alexandrovna e FERRAZ-MELLO, Sylvio. Dynamics of two planets in the 2:1 and 3:2 mean motion resonances. Bulletin of the American Astronomical Society, v. 34, n. 3, p. 892, 2002Tradução . . Acesso em: 04 mar. 2026. -
APA
Callegari Jr., N., Michtchenko, T. A., & Ferraz-Mello, S. (2002). Dynamics of two planets in the 2:1 and 3:2 mean motion resonances. Bulletin of the American Astronomical Society, 34( 3), 892. -
NLM
Callegari Jr. N, Michtchenko TA, Ferraz-Mello S. Dynamics of two planets in the 2:1 and 3:2 mean motion resonances. Bulletin of the American Astronomical Society. 2002 ; 34( 3): 892.[citado 2026 mar. 04 ] -
Vancouver
Callegari Jr. N, Michtchenko TA, Ferraz-Mello S. Dynamics of two planets in the 2:1 and 3:2 mean motion resonances. Bulletin of the American Astronomical Society. 2002 ; 34( 3): 892.[citado 2026 mar. 04 ] - Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects
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