Dynamics of two planets in the 2:1 and 3:2 mean motion resonances (2002)
Source: Bulletin of the American Astronomical Society. Unidade: IAG
Assunto: SISTEMA SOLAR
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: 21 maio 2024.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 2024 maio 21 ]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 2024 maio 21 ]