Filtros : "IAG" "França" "Barros, D. A" Limpar

Filtros



Refine with date range


  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: GALÁXIAS, GALÁXIA (VIA LÁCTEA)

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      MICHTCHENKO, Tatiana Alexandrovna et al. Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model. Astronomy and Astrophysysics, v. 597, p. A39, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628895. Acesso em: 16 out. 2024.
    • APA

      Michtchenko, T. A., Vieira, R. S. S., Barros, D. A., & Lépine, J. R. D. (2017). Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model. Astronomy and Astrophysysics, 597, A39. doi:10.1051/0004-6361/201628895
    • NLM

      Michtchenko TA, Vieira RSS, Barros DA, Lépine JRD. Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model [Internet]. Astronomy and Astrophysysics. 2017 ;597 A39.[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628895
    • Vancouver

      Michtchenko TA, Vieira RSS, Barros DA, Lépine JRD. Modelling resonances and orbital chaos in disk galaxies - Application to a Milky Way spiral model [Internet]. Astronomy and Astrophysysics. 2017 ;597 A39.[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628895
  • Source: Astronomy & Astronomy. Unidade: IAG

    Subjects: ESTRUTURA DA GALÁXIA, GALÁXIA (VIA LÁCTEA)

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      BARROS, D. A e LÉPINE, Jacques Raymond Daniel e DIAS, W S. Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk. Astronomy & Astronomy, v. 593, n. 108, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527535. Acesso em: 16 out. 2024.
    • APA

      Barros, D. A., Lépine, J. R. D., & Dias, W. S. (2016). Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk. Astronomy & Astronomy, 593( 108). doi:10.1051/0004-6361/201527535
    • NLM

      Barros DA, Lépine JRD, Dias WS. Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk [Internet]. Astronomy & Astronomy. 2016 ;593( 108):[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527535
    • Vancouver

      Barros DA, Lépine JRD, Dias WS. Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk [Internet]. Astronomy & Astronomy. 2016 ;593( 108):[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527535
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), DINÂMICA DA GALÁXIA, ESTRUTURA DA GALÁXIA, GALÁXIAS ESPIRAIS

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      JUNQUEIRA, T. C et al. A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy. Astronomy & Astrophysics, v. 550, p. A91/1-A91/12, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201219769. Acesso em: 16 out. 2024.
    • APA

      Junqueira, T. C., Lépine, J. R. D., Braga, C. A. S., & Barros, D. A. (2013). A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy. Astronomy & Astrophysics, 550, A91/1-A91/12. doi:10.1051/0004-6361/201219769
    • NLM

      Junqueira TC, Lépine JRD, Braga CAS, Barros DA. A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy [Internet]. Astronomy & Astrophysics. 2013 ; 550 A91/1-A91/12.[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201219769
    • Vancouver

      Junqueira TC, Lépine JRD, Braga CAS, Barros DA. A new model for gravitational potential perturbations in disks of spiral galaxies: an application to our Galaxy [Internet]. Astronomy & Astrophysics. 2013 ; 550 A91/1-A91/12.[citado 2024 out. 16 ] Available from: https://doi.org/10.1051/0004-6361/201219769
  • Source: LARIM 2013: Abstract Book. Conference titles: Latin American Rgional IAU Meeting. Unidade: IAG

    Subjects: GALÁXIAS ESPIRAIS, GALÁXIA (VIA LÁCTEA)

    How to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      LÉPINE, Jacques Raymond Daniel et al. The role of the corotation resonance in the secular evolution of disks of spiral galaxies. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 16 out. 2024.
    • APA

      Lépine, J. R. D., Scarano Júnior, S., Barros, D. A., Junqueira, T. C., Dias, W. S., & Andrievsky, S. (2013). The role of the corotation resonance in the secular evolution of disks of spiral galaxies. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
    • NLM

      Lépine JRD, Scarano Júnior S, Barros DA, Junqueira TC, Dias WS, Andrievsky S. The role of the corotation resonance in the secular evolution of disks of spiral galaxies. LARIM 2013: Abstract Book. 2013 ;[citado 2024 out. 16 ]
    • Vancouver

      Lépine JRD, Scarano Júnior S, Barros DA, Junqueira TC, Dias WS, Andrievsky S. The role of the corotation resonance in the secular evolution of disks of spiral galaxies. LARIM 2013: Abstract Book. 2013 ;[citado 2024 out. 16 ]

Digital Library of Intellectual Production of Universidade de São Paulo     2012 - 2024