The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis (2006)
- Authors:
- Autor USP: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG
- Unidade: IAG
- DOI: 10.1051/0004-6361:20065518
- Subjects: ESPECTROSCOPIA; PLANETAS MENORES; ASTEROIDES
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v. 459, n. 3, p. 969-976, 2006
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
ALVAREZ-CANDAL, A et al. The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis. Astronomy and Astrophysics, v. 459, n. 3, p. 969-976, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065518. Acesso em: 23 abr. 2024. -
APA
Alvarez-Candal, A., Duffard, R., Lazzaro, D., & Michtchenko, T. A. (2006). The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis. Astronomy and Astrophysics, 459( 3), 969-976. doi:10.1051/0004-6361:20065518 -
NLM
Alvarez-Candal A, Duffard R, Lazzaro D, Michtchenko TA. The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis [Internet]. Astronomy and Astrophysics. 2006 ; 459( 3): 969-976.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1051/0004-6361:20065518 -
Vancouver
Alvarez-Candal A, Duffard R, Lazzaro D, Michtchenko TA. The inner region of the asteroid Main Belt: a spectroscopic and dynamic analysis [Internet]. Astronomy and Astrophysics. 2006 ; 459( 3): 969-976.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1051/0004-6361:20065518 - On the V-type asteroids outside the Vesta family: is(21238)1995 WV7 a former member of the Eunomia family?
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- Probing the nature of the Baptistina Family
- Angular momentum exchange during secular migration of two-planet systems
- Elaboração de um cenário para formação de planetas gigantes
- On the current distribution of the main belt objects:: constraints for the evolutionary models
- Secular dynamics of the three-body problem: application to the "úpsilon" Andromedae planetary system
- 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
- Primordial migration of co-orbital satellites as a mechanism for the horseshoe orbit of Janus –Epimetheus
Informações sobre o DOI: 10.1051/0004-6361:20065518 (Fonte: oaDOI API)
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