Filtros : "Carvano, J. M" Limpar

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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: PLANETAS MENORES, ASTEROIDES, ANÁLISE DE DADOS, MECÂNICA CELESTE

    Acesso à fonteDOIHow to cite
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    • ABNT

      MICHTCHENKO, Tatiana Alexandrovna e LAZZARO, D e CARVANO, J. M. On the current distribution of main belt objects: constraints for evolutionary models. Astronomy & Astrophysics, v. 588, p. A11/1-A11/26, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525754. Acesso em: 27 abr. 2024.
    • APA

      Michtchenko, T. A., Lazzaro, D., & Carvano, J. M. (2016). On the current distribution of main belt objects: constraints for evolutionary models. Astronomy & Astrophysics, 588, A11/1-A11/26. doi:10.1051/0004-6361/201525754
    • NLM

      Michtchenko TA, Lazzaro D, Carvano JM. On the current distribution of main belt objects: constraints for evolutionary models [Internet]. Astronomy & Astrophysics. 2016 ; 588 A11/1-A11/26.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201525754
    • Vancouver

      Michtchenko TA, Lazzaro D, Carvano JM. On the current distribution of main belt objects: constraints for evolutionary models [Internet]. Astronomy & Astrophysics. 2016 ; 588 A11/1-A11/26.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201525754
  • Source: EPSC Abstracts. Conference titles: EPSC-DPS Joint Meeting 2011. Unidade: IAG

    Subjects: ASTEROIDES, MECÂNICA CELESTE

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    • ABNT

      MICHTCHENKO, Tatiana Alexandrovna et al. Dynamic picture of the main asteroid belt. 2011, Anais.. Toulouse: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 2011. . Acesso em: 27 abr. 2024.
    • APA

      Michtchenko, T. A., Lazzaro, D., Carvano, J. M., & Mothé-Diniz, T. (2011). Dynamic picture of the main asteroid belt. In EPSC Abstracts (Vol. 6). Toulouse: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
    • NLM

      Michtchenko TA, Lazzaro D, Carvano JM, Mothé-Diniz T. Dynamic picture of the main asteroid belt. EPSC Abstracts. 2011 ; 6[citado 2024 abr. 27 ]
    • Vancouver

      Michtchenko TA, Lazzaro D, Carvano JM, Mothé-Diniz T. Dynamic picture of the main asteroid belt. EPSC Abstracts. 2011 ; 6[citado 2024 abr. 27 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS MENORES, ASTEROIDES

    Acesso à fonteDOIHow to cite
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    • 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: 27 abr. 2024.
    • 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 2024 abr. 27 ] 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 2024 abr. 27 ] Available from: https://doi.org/10.1111/j.1365-2966.2009.15825.x
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Assunto: SISTEMA SOLAR

    Acesso à fonteDOIHow to cite
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    • ABNT

      CARVANO, J. M e FERRAZ-MELLO, Sylvio e LAZZARO, D. Physical and dynamical characterization of (5201) Ferraz-Mello, a possible extinct Jupiter family comet. Astronomy & Astrophysics, v. 489, p. 811-817, 2008Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:200809820. Acesso em: 27 abr. 2024.
    • APA

      Carvano, J. M., Ferraz-Mello, S., & Lazzaro, D. (2008). Physical and dynamical characterization of (5201) Ferraz-Mello, a possible extinct Jupiter family comet. Astronomy & Astrophysics, 489, 811-817. doi:10.1051/0004-6361:200809820
    • NLM

      Carvano JM, Ferraz-Mello S, Lazzaro D. Physical and dynamical characterization of (5201) Ferraz-Mello, a possible extinct Jupiter family comet [Internet]. Astronomy & Astrophysics. 2008 ;489 811-817.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361:200809820
    • Vancouver

      Carvano JM, Ferraz-Mello S, Lazzaro D. Physical and dynamical characterization of (5201) Ferraz-Mello, a possible extinct Jupiter family comet [Internet]. Astronomy & Astrophysics. 2008 ;489 811-817.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361:200809820

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