Reliability of orbital fits for resonant extrasolar planetary systems: the case of HD82943 (2008)
- Authors:
- USP affiliated authors: MELLO, SYLVIO FERRAZ DE - IAG ; MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- DOI: 10.1111/j.1365-2966.2008.12979.x
- Subjects: MECÂNICA CELESTE; SISTEMA SOLAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 385, n. 4, p. 2151-2160, 2008
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
BEAUGÉ, C; GIUPPONE, C. A; FERRAZ-MELLO, Sylvio; MICHTCHENKO, Tatiana Alexandrovna. Reliability of orbital fits for resonant extrasolar planetary systems: the case of HD82943. Monthly Notices of the Royal Astronomical Society, Oxford, v. 385, n. 4, p. 2151-2160, 2008. DOI: 10.1111/j.1365-2966.2008.12979.x. -
APA
Beaugé, C., Giuppone, C. A., Ferraz-Mello, S., & Michtchenko, T. A. (2008). Reliability of orbital fits for resonant extrasolar planetary systems: the case of HD82943. Monthly Notices of the Royal Astronomical Society, 385( 4), 2151-2160. doi:10.1111/j.1365-2966.2008.12979.x -
NLM
Beaugé C, Giuppone CA, Ferraz-Mello S, Michtchenko TA. Reliability of orbital fits for resonant extrasolar planetary systems: the case of HD82943. Monthly Notices of the Royal Astronomical Society. 2008 ; 385( 4): 2151-2160. -
Vancouver
Beaugé C, Giuppone CA, Ferraz-Mello S, Michtchenko TA. Reliability of orbital fits for resonant extrasolar planetary systems: the case of HD82943. Monthly Notices of the Royal Astronomical Society. 2008 ; 385( 4): 2151-2160. - On the depletion of the Hecuba gap in the asteroidal belt
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- Retrato dinâmico do cinturão asteroidal interior
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- Planetary masses and orbital parameters from radial velocity measurements
- Dynamic portrait of the planetary 2/1 mean-motion resonace: II. systems with a more massive inner planet
- Origin of the Basaltic Asteroid 1459 Magnya: A Dynamical and Mineralogical Study of the Outer Main Belt
- Dynamics of two planets in the 2:1 and 3:2 mean motion resonances
Informações sobre o DOI: 10.1111/j.1365-2966.2008.12979.x (Fonte: oaDOI API)
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