Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12 (2006)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- Subjects: CAOS (SISTEMAS DINÂMICOS); PLANETAS; PULSARES; SISTEMA SOLAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Celestial Mechanics and Dynamical Astronomy
- ISSN: 0923-2958
- Volume/Número/Paginação/Ano: v. 94, n. 4, p. 381-397, 2006
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ABNT
CALLEGARI JÚNIOR, Nelson e FERRAZ-MELLO, Sylvio e MICHTCHENKO, Tatiana Alexandrovna. Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy, v. 94, n. 4, p. 381-397, 2006Tradução . . Acesso em: 21 maio 2024. -
APA
Callegari Júnior, N., Ferraz-Mello, S., & Michtchenko, T. A. (2006). Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy, 94( 4), 381-397. -
NLM
Callegari Júnior N, Ferraz-Mello S, Michtchenko TA. Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy. 2006 ; 94( 4): 381-397.[citado 2024 maio 21 ] -
Vancouver
Callegari Júnior N, Ferraz-Mello S, Michtchenko TA. Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12. Celestial Mechanics and Dynamical Astronomy. 2006 ; 94( 4): 381-397.[citado 2024 maio 21 ] - Planetary masses and orbital parameters from radial velocity measurements
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