Filtros : "EACH" "IAG-AGA" "Estados Unidos" Removidos: "GEOCIÊNCIAS" "CIÊNCIA POLÍTICA E RELAÇÕES INTERNACIONAIS / B3" "Aramo, Carla" Limpar

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  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Assunto: ASTROFÍSICA

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    • ABNT

      TORREJÓN, Tania Elizabeth Medina e PINO, Elisabete Maria de Gouveia Dal e KOWAL, Grzegorz. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales. The Astrophysical Journal, v. 952, n. 2, p. 01-11, 2023Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/acd699. Acesso em: 30 jul. 2024.
    • APA

      Torrejón, T. E. M., Pino, E. M. de G. D., & Kowal, G. (2023). Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales. The Astrophysical Journal, 952( 2), 01-11. doi:10.3847/1538-4357/acd699
    • NLM

      Torrejón TEM, Pino EM de GD, Kowal G. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales [Internet]. The Astrophysical Journal. 2023 ; 952( 2): 01-11.[citado 2024 jul. 30 ] Available from: https://doi.org/10.3847/1538-4357/acd699
    • Vancouver

      Torrejón TEM, Pino EM de GD, Kowal G. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales [Internet]. The Astrophysical Journal. 2023 ; 952( 2): 01-11.[citado 2024 jul. 30 ] Available from: https://doi.org/10.3847/1538-4357/acd699
  • Source: Physical Review D. Unidades: EACH, IAG, IF

    Assunto: BURACOS NEGROS

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      FIRAVITOVA, Fabian Ruiz e MENDES, Carlos Molina e LIMA, Jose Ademir Sales de. Dynamical model for primordial black holes. Physical Review D, v. 102, 2020Tradução . . Disponível em: https://doi.org/10.1103/PhysRevD.102.123516. Acesso em: 30 jul. 2024.
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      Firavitova, F. R., Mendes, C. M., & Lima, J. A. S. de. (2020). Dynamical model for primordial black holes. Physical Review D, 102. doi:10.1103/PhysRevD.102.123516
    • NLM

      Firavitova FR, Mendes CM, Lima JAS de. Dynamical model for primordial black holes [Internet]. Physical Review D. 2020 ; 102[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/PhysRevD.102.123516
    • Vancouver

      Firavitova FR, Mendes CM, Lima JAS de. Dynamical model for primordial black holes [Internet]. Physical Review D. 2020 ; 102[citado 2024 jul. 30 ] Available from: https://doi.org/10.1103/PhysRevD.102.123516
  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Subjects: PLASMA, ONDAS DE CHOQUE, CAMPO MAGNÉTICO, SOL

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      PÁEZ, A. et al. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration. The Astrophysical Journal, v. 879, n. 2, p. 01-09, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab2460. Acesso em: 30 jul. 2024.
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      Páez, A., Jatenco-Pereira, V., Gonçalves, D. A. F., & Opher, M. (2019). Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration. The Astrophysical Journal, 879( 2), 01-09. doi:10.3847/1538-4357/ab2460
    • NLM

      Páez A, Jatenco-Pereira V, Gonçalves DAF, Opher M. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration [Internet]. The Astrophysical Journal. 2019 ; 879( 2): 01-09.[citado 2024 jul. 30 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
    • Vancouver

      Páez A, Jatenco-Pereira V, Gonçalves DAF, Opher M. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration [Internet]. The Astrophysical Journal. 2019 ; 879( 2): 01-09.[citado 2024 jul. 30 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
  • Source: The Astrophysical Journal: an international review of astronomy and astronomical physics. Unidades: EACH, IAG

    Subjects: VENTO SOLAR, SOL, CAMPO MAGNÉTICO, ATIVIDADE SOLAR

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      MURCIA, Miguel Andres Paez et al. Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces. The Astrophysical Journal: an international review of astronomy and astronomical physics, v. 851, p. 01-09, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa9753. Acesso em: 30 jul. 2024.
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      Murcia, M. A. P., Pereira, V. J. S., Gonçalves, D. A. F., & opher, merav. (2017). Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces. The Astrophysical Journal: an international review of astronomy and astronomical physics, 851, 01-09. doi:10.3847/1538-4357/aa9753
    • NLM

      Murcia MAP, Pereira VJS, Gonçalves DAF, opher merav. Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces [Internet]. The Astrophysical Journal: an international review of astronomy and astronomical physics. 2017 ; 851 01-09.[citado 2024 jul. 30 ] Available from: https://doi.org/10.3847/1538-4357/aa9753
    • Vancouver

      Murcia MAP, Pereira VJS, Gonçalves DAF, opher merav. Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces [Internet]. The Astrophysical Journal: an international review of astronomy and astronomical physics. 2017 ; 851 01-09.[citado 2024 jul. 30 ] Available from: https://doi.org/10.3847/1538-4357/aa9753
  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Subjects: AGLOMERADOS DE GALÁXIAS, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, TURBULÊNCIA

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      SANTOS-LIMA, R et al. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium. The Astrophysical Journal, v. 781, n. 84, p. 1-21, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/781/2/84. Acesso em: 30 jul. 2024.
    • APA

      Santos-Lima, R., Dal Pino, E. M. de G., Kowal, G., Falceta-Gonçalves, D., Lazarian, A., & Nakwacki, M. S. (2014). Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium. The Astrophysical Journal, 781( 84), 1-21. doi:10.1088/0004-637X/781/2/84
    • NLM

      Santos-Lima R, Dal Pino EM de G, Kowal G, Falceta-Gonçalves D, Lazarian A, Nakwacki MS. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium [Internet]. The Astrophysical Journal. 2014 ;781( 84): 1-21.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
    • Vancouver

      Santos-Lima R, Dal Pino EM de G, Kowal G, Falceta-Gonçalves D, Lazarian A, Nakwacki MS. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium [Internet]. The Astrophysical Journal. 2014 ;781( 84): 1-21.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Subjects: GALÁXIAS, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, TURBULÊNCIA

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    • ABNT

      SANTOS-LIMA, R et al. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium. The Astrophysical Journal, v. 781, n. 2, p. 1-21, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/781/2/84. Acesso em: 30 jul. 2024.
    • APA

      Santos-Lima, R., Dal Pino, E. M. de G., Kowal, G., Falceta Gonçalves, D. A., Lazarian, A., & Nakwacki, M. S. (2014). Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium. The Astrophysical Journal, 781( 2), 1-21. doi:10.1088/0004-637X/781/2/84
    • NLM

      Santos-Lima R, Dal Pino EM de G, Kowal G, Falceta Gonçalves DA, Lazarian A, Nakwacki MS. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium [Internet]. The Astrophysical Journal. 2014 ; 781( 2): 1-21.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
    • Vancouver

      Santos-Lima R, Dal Pino EM de G, Kowal G, Falceta Gonçalves DA, Lazarian A, Nakwacki MS. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium [Internet]. The Astrophysical Journal. 2014 ; 781( 2): 1-21.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), TURBULÊNCIA

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      POIDEVIN, Frédérick et al. Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog. The Astrophysical Journal, v. 777, p. 112/1-112/15, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/777/2/112. Acesso em: 30 jul. 2024.
    • APA

      Poidevin, F., Falceta Gonçalves, D. A., Kowal, G., Dal Pino, E. M. de G., & Magalhães, A. M. (2013). Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog. The Astrophysical Journal, 777, 112/1-112/15. doi:10.1088/0004-637X/777/2/112
    • NLM

      Poidevin F, Falceta Gonçalves DA, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog [Internet]. The Astrophysical Journal. 2013 ; 777 112/1-112/15.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1088/0004-637X/777/2/112
    • Vancouver

      Poidevin F, Falceta Gonçalves DA, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog [Internet]. The Astrophysical Journal. 2013 ; 777 112/1-112/15.[citado 2024 jul. 30 ] Available from: https://doi.org/10.1088/0004-637X/777/2/112
  • Source: The Astronomical Journal. Unidades: EACH, IAG

    Subjects: GALAXIA, ESTRELAS

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      ORTIZ, Roberto et al. A search for field horizontal-branch stars near the south galactic pole. The Astronomical Journal, v. 139, p. 1031-1044, 2010Tradução . . Acesso em: 30 jul. 2024.
    • APA

      Ortiz, R., Wilhelm, R., Costa, R. D. 'A. D. da, Rossi, S. C. F., & Beers, T. C. (2010). A search for field horizontal-branch stars near the south galactic pole. The Astronomical Journal, 139, 1031-1044.
    • NLM

      Ortiz R, Wilhelm R, Costa RD'AD da, Rossi SCF, Beers TC. A search for field horizontal-branch stars near the south galactic pole. The Astronomical Journal. 2010 ; 139 1031-1044.[citado 2024 jul. 30 ]
    • Vancouver

      Ortiz R, Wilhelm R, Costa RD'AD da, Rossi SCF, Beers TC. A search for field horizontal-branch stars near the south galactic pole. The Astronomical Journal. 2010 ; 139 1031-1044.[citado 2024 jul. 30 ]
  • Source: The Astronomical Journal. Unidades: EACH, IAG

    Subjects: GALÁXIAS, ESTRELAS

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      ORTIZ, R. et al. A survey of Early-Type Stars based on the two micron all sky survey database. The Astronomical Journal, v. 134, n. 3, p. 1183-1194, 2007Tradução . . Acesso em: 30 jul. 2024.
    • APA

      Ortiz, R., Malacarne, M., Wilhelm, R., Costa, R. D. D., Rossi, S., Maciel, W. J., & Costa, A. F. M. (2007). A survey of Early-Type Stars based on the two micron all sky survey database. The Astronomical Journal, 134( 3), 1183-1194.
    • NLM

      Ortiz R, Malacarne M, Wilhelm R, Costa RDD, Rossi S, Maciel WJ, Costa AFM. A survey of Early-Type Stars based on the two micron all sky survey database. The Astronomical Journal. 2007 ; 134( 3): 1183-1194.[citado 2024 jul. 30 ]
    • Vancouver

      Ortiz R, Malacarne M, Wilhelm R, Costa RDD, Rossi S, Maciel WJ, Costa AFM. A survey of Early-Type Stars based on the two micron all sky survey database. The Astronomical Journal. 2007 ; 134( 3): 1183-1194.[citado 2024 jul. 30 ]

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