Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects (2010)
- Authors:
- USP affiliated authors: MICHTCHENKO, TATIANA ALEXANDROVNA - IAG ; MELLO, SYLVIO FERRAZ DE - IAG
- Unidade: IAG
- DOI: 10.1111/j.1365-2966.2009.15825.x
- Subjects: PLANETAS MENORES; ASTEROIDES
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 401, n. 4, p. 2499-2516, 2010
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
MICHTCHENKO, Tatiana Alexandrovna et al. Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects. Monthly Notices of the Royal Astronomical Society, v. 401, n. 4, p. 2499-2516, 2010Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2009.15825.x. Acesso em: 12 jan. 2026. -
APA
Michtchenko, T. A., Lazzaro, D., Carvano, J. M., & Ferraz-Mello, S. (2010). Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects. Monthly Notices of the Royal Astronomical Society, 401( 4), 2499-2516. doi:10.1111/j.1365-2966.2009.15825.x -
NLM
Michtchenko TA, Lazzaro D, Carvano JM, Ferraz-Mello S. Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects [Internet]. Monthly Notices of the Royal Astronomical Society. 2010 ; 401( 4): 2499-2516.[citado 2026 jan. 12 ] Available from: https://doi.org/10.1111/j.1365-2966.2009.15825.x -
Vancouver
Michtchenko TA, Lazzaro D, Carvano JM, Ferraz-Mello S. Dynamic picture of the inner asteroid belt: implications for the density, size and taxonomic distributions of real objects [Internet]. Monthly Notices of the Royal Astronomical Society. 2010 ; 401( 4): 2499-2516.[citado 2026 jan. 12 ] Available from: https://doi.org/10.1111/j.1365-2966.2009.15825.x - Tidal evolution of a close-in planet with a more massive outer companion
- Orbital evolution of asteroids in the hecuba gap
- Evolution of migrating planet pairs in resonance
- Dynamics of two planets in the 3/2 mean-motion resonance: application to the planetary system of the pulsar PSR B1257+12
- Modeling close encouters with massive asteroids: a Markovian approach. An aplication to the Vesta family
- Stationary orbits in resonant extrasolar planetary systems
- Resonances and stability of extra-solar planetary systems
- The role of close encounters with (4) Vesta in the origin of the basaltic NEAs
- Secular behavior of a pair of coplanar planets
- Modeling the 3-D secular planetary three-body problem discussion on the outer 'úpsilon' Andromedae planetary system
Informações sobre o DOI: 10.1111/j.1365-2966.2009.15825.x (Fonte: oaDOI API)
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