A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances (2009)
- Autores:
- Autor USP: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- Assuntos: PLANETAS MENORES; ASTEROIDES; MECÂNICA CELESTE
- Idioma: Inglês
- Imprenta:
- Fonte:
- Título do periódico: Astronomy & Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v. 493, p. 267-282, 2009
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ABNT
CARRUBA, V e MICHTCHENKO, Tatiana Alexandrovna. A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics, v. 493, p. 267-282, 2009Tradução . . Acesso em: 19 abr. 2024. -
APA
Carruba, V., & Michtchenko, T. A. (2009). A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics, 493, 267-282. -
NLM
Carruba V, Michtchenko TA. A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics. 2009 ; 493 267-282.[citado 2024 abr. 19 ] -
Vancouver
Carruba V, Michtchenko TA. A frequency approach to identifying asteroid families: II. Families interacting with nonlinear secular resonances and low-order mean-motion resonances. Astronomy & Astrophysics. 2009 ; 493 267-282.[citado 2024 abr. 19 ] - On the V-type asteroids outside the Vesta family: is(21238)1995 WV7 a former member of the Eunomia family?
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- Discovery of a basaltic asteroid in the outer main belt
- The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis
- Primordial migration of co-orbital satellites as a mechanism for the horseshoe orbit of Janus –Epimetheus
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