Modelling the secular evolution of migrating planet pairs (2011)
- Authors:
- Autor USP: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- DOI: 10.1111/j.1365-2966.2011.18857.x
- Subjects: MECÂNICA CELESTE; PLANETAS; SATÉLITES
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 415, p. 2275-2292, 2011
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
-
ABNT
MICHTCHENKO, Tatiana Alexandrovna e RODRÍGUEZ, A. Modelling the secular evolution of migrating planet pairs. Monthly Notices of the Royal Astronomical Society, v. 415, p. 2275-2292, 2011Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2011.18857.x. Acesso em: 19 abr. 2024. -
APA
Michtchenko, T. A., & Rodríguez, A. (2011). Modelling the secular evolution of migrating planet pairs. Monthly Notices of the Royal Astronomical Society, 415, 2275-2292. doi:10.1111/j.1365-2966.2011.18857.x -
NLM
Michtchenko TA, Rodríguez A. Modelling the secular evolution of migrating planet pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2011 ; 415 2275-2292.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1111/j.1365-2966.2011.18857.x -
Vancouver
Michtchenko TA, Rodríguez A. Modelling the secular evolution of migrating planet pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2011 ; 415 2275-2292.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1111/j.1365-2966.2011.18857.x - On the V-type asteroids outside the Vesta family: is(21238)1995 WV7 a former member of the Eunomia family?
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- A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances
- Discovery of a basaltic asteroid in the outer main belt
- The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis
Informações sobre o DOI: 10.1111/j.1365-2966.2011.18857.x (Fonte: oaDOI API)
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