Filtros : "CAMPO MAGNÉTICO" "IAG-AGA" Removido: "Alcaniz, J. S" Limpar

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  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: HIDRODINÂMICA, CAMPO MAGNÉTICO, ESTRELAS, POLARIZAÇÃO (ASTRONOMIA)

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      MUNOZ, M S et al. Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model. Monthly Notices of the Royal Astronomical Society, v. 511, p. 3228-3249, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3767. Acesso em: 24 jul. 2024.
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      Munoz, M. S., Wade G A,, Faes, D. M., Carciofi, A. C., & Labadie-Bartz, J. (2022). Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model. Monthly Notices of the Royal Astronomical Society, 511, 3228-3249. doi:10.1093/mnras/stab3767
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      Munoz MS, Wade G A, Faes DM, Carciofi AC, Labadie-Bartz J. Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 511 3228-3249.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stab3767
    • Vancouver

      Munoz MS, Wade G A, Faes DM, Carciofi AC, Labadie-Bartz J. Untangling magnetic massive star properties with linear polarization variability and the analytic dynamical magnetosphere model [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 511 3228-3249.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stab3767
  • Fonte: Astrophysical Journal Supplement Series. Unidade: IAG

    Assuntos: POEIRA INTERESTELAR, CAMPO MAGNÉTICO

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      FRISCH, P. C e PIIROLA, V. e MAGALHÃES, Antonio Mário. Whence the interstellar magnetic field shaping the heliosphere?. Astrophysical Journal Supplement Series, v. 259, p. 48, 2022Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/ac5750. Acesso em: 24 jul. 2024.
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      Frisch, P. C., Piirola, V., & Magalhães, A. M. (2022). Whence the interstellar magnetic field shaping the heliosphere? Astrophysical Journal Supplement Series, 259, 48. doi:10.3847/1538-4365/ac5750
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      Frisch PC, Piirola V, Magalhães AM. Whence the interstellar magnetic field shaping the heliosphere? [Internet]. Astrophysical Journal Supplement Series. 2022 ; 259 48.[citado 2024 jul. 24 ] Available from: https://doi.org/10.3847/1538-4365/ac5750
    • Vancouver

      Frisch PC, Piirola V, Magalhães AM. Whence the interstellar magnetic field shaping the heliosphere? [Internet]. Astrophysical Journal Supplement Series. 2022 ; 259 48.[citado 2024 jul. 24 ] Available from: https://doi.org/10.3847/1538-4365/ac5750
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: CAMPO MAGNÉTICO

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      SANTOS-LIMA, R et al. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, v. 503, p. 1290-1309, 2021Tradução . . Disponível em: https://academic.oup.com/mnras/article/503/1/1290/6144594. Acesso em: 24 jul. 2024.
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      Santos-Lima, R., Guerrero, G., Dal Pino, E. M. de G., & Lazarian, A. (2021). Diffusion of large-scale magnetic fields by reconnection in MHD turbulence. Monthly Notices of the Royal Astronomical Society, 503, 1290-1309. doi:10.1093/mnras/stab470
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      Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2024 jul. 24 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
    • Vancouver

      Santos-Lima R, Guerrero G, Dal Pino EM de G, Lazarian A. Diffusion of large-scale magnetic fields by reconnection in MHD turbulence [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 503 1290-1309.[citado 2024 jul. 24 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, ESTRUTURA DA GALÁXIA

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      LEAMAN, Ryan e COELHO, Paula Rodrigues Teixeira. Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA. Monthly Notices of the Royal Astronomical Society, v. 488, n. 3, p. 3904-3928, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz1844. Acesso em: 24 jul. 2024.
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      Leaman, R., & Coelho, P. R. T. (2019). Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA. Monthly Notices of the Royal Astronomical Society, 488( 3), 3904-3928. doi:10.1093/mnras/stz1844
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      Leaman R, Coelho PRT. Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 488( 3): 3904-3928.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stz1844
    • Vancouver

      Leaman R, Coelho PRT. Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 488( 3): 3904-3928.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stz1844
  • Fonte: The Astrophysical Journal. Unidades: IAG, EACH

    Assuntos: 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: 24 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
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      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. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
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      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. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, RAIOS GAMA

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      BATISTA, Rafael Alves e SAVELIEV, Andrey e DAL PINO, Elisabete Maria de Gouveia. The impact of plasma instabilities on the spectra of TeV blazars. Monthly Notices of the Royal Astronomical Society, v. 489, n. 3, p. 3836-3849, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2389. Acesso em: 24 jul. 2024.
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      Batista, R. A., Saveliev, A., & Dal Pino, E. M. de G. (2019). The impact of plasma instabilities on the spectra of TeV blazars. Monthly Notices of the Royal Astronomical Society, 489( 3), 3836-3849. doi:10.1093/mnras/stz2389
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      Batista RA, Saveliev A, Dal Pino EM de G. The impact of plasma instabilities on the spectra of TeV blazars [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 3): 3836-3849.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stz2389
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      Batista RA, Saveliev A, Dal Pino EM de G. The impact of plasma instabilities on the spectra of TeV blazars [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 3): 3836-3849.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stz2389
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR

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    • ABNT

      GUERRERO, G et al. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?. The Astrophysical Journal, v. 880, n. 1, p. 6/1-6/20, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab224a. Acesso em: 24 jul. 2024.
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      Guerrero, G., Zaire, B., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2019). What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? The Astrophysical Journal, 880( 1), 6/1-6/20. doi:10.3847/1538-4357/ab224a
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      Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jul. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
    • Vancouver

      Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2024 jul. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
  • Fonte: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Assuntos: DISCOS DE ACRESÇÃO, CAMPO MAGNÉTICO

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      MENDES, Camile et al. Magnetic field decay in black widow pulsars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 475, p. 2178-2184, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx3319. Acesso em: 24 jul. 2024.
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      Mendes, C., Avellar, M. G. B. de, Horvath, J. E., Souza, R. A. de, Benvenuto, O. G., & De Vito, M. A. (2018). Magnetic field decay in black widow pulsars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 475, 2178-2184. doi:10.1093/mnras/stx3319
    • NLM

      Mendes C, Avellar MGB de, Horvath JE, Souza RA de, Benvenuto OG, De Vito MA. Magnetic field decay in black widow pulsars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;475 2178-2184.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stx3319
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      Mendes C, Avellar MGB de, Horvath JE, Souza RA de, Benvenuto OG, De Vito MA. Magnetic field decay in black widow pulsars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;475 2178-2184.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stx3319
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH

    Assuntos: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS, MEIO INTERESTELAR

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      SANTOS-LIMA, Reinaldo et al. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback. Monthly Notices of the Royal Astronomical Society, v. 465, n. 4, p. 4866-4871, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw3050. Acesso em: 24 jul. 2024.
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      Santos-Lima, R., Dal Pino, E. M. de G., Falceta Gonçalves, D. A., Nakwacki, M. S., & Kowal, G. (2017). Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback. Monthly Notices of the Royal Astronomical Society, 465( 4), 4866-4871. doi:10.1093/mnras/stw3050
    • NLM

      Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA, Nakwacki MS, Kowal G. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 465( 4): 4866-4871.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stw3050
    • Vancouver

      Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA, Nakwacki MS, Kowal G. Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 465( 4): 4866-4871.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stw3050
  • Fonte: The Astrophysical Journal: an international review of astronomy and astronomical physics. Unidades: EACH, IAG

    Assuntos: 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: 24 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
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      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. 24 ] 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. 24 ] Available from: https://doi.org/10.3847/1538-4357/aa9753
  • Fonte: The lives and death-throes of massive stars: proceedings of the 329th symposium of the International Astronomical Union held in Auckland, New Zealand November 28- December 2, 2016. Nome do evento: IAU SYMPOSIUM. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), ESPECTROSCOPIA

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      RUBINHO, Marcelo Soares et al. HD151018: strong magnetic field in a giant O-type star? 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003477. Acesso em: 24 jul. 2024.
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      Rubinho, M. S., Damineli Neto, A., Carciofi, A. C., & Moser, D. (2017). HD151018: strong magnetic field in a giant O-type star? In The lives and death-throes of massive stars: proceedings of the 329th symposium of the International Astronomical Union held in Auckland, New Zealand November 28- December 2, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317003477
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      Rubinho MS, Damineli Neto A, Carciofi AC, Moser D. HD151018: strong magnetic field in a giant O-type star? [Internet]. The lives and death-throes of massive stars: proceedings of the 329th symposium of the International Astronomical Union held in Auckland, New Zealand November 28- December 2, 2016. 2017 ;[citado 2024 jul. 24 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003477
    • Vancouver

      Rubinho MS, Damineli Neto A, Carciofi AC, Moser D. HD151018: strong magnetic field in a giant O-type star? [Internet]. The lives and death-throes of massive stars: proceedings of the 329th symposium of the International Astronomical Union held in Auckland, New Zealand November 28- December 2, 2016. 2017 ;[citado 2024 jul. 24 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003477
  • Fonte: Astrophysical Journal Letters. Unidade: IAG

    Assuntos: SOL, CAMPO MAGNÉTICO

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      GUERRERO, G e SMOLARKIEWICZ, P. K e DAL PINO, Elisabete Maria de Gouveia. Understanding solar torsional oscillations from global dynamo models. Astrophysical Journal Letters, 2016Tradução . . Disponível em: https://arxiv.org/abs/1608.02278. Acesso em: 24 jul. 2024.
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      Guerrero, G., Smolarkiewicz, P. K., & Dal Pino, E. M. de G. (2016). Understanding solar torsional oscillations from global dynamo models. Astrophysical Journal Letters. doi:10.3847/2041-8205/828/1/L3
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      Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 jul. 24 ] Available from: https://arxiv.org/abs/1608.02278
    • Vancouver

      Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 jul. 24 ] Available from: https://arxiv.org/abs/1608.02278
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: ESTRELAS, INSTRUMENTAÇÃO (ASTRONOMIA), CAMPO MAGNÉTICO

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      WADE, G. A et al. The MiMeS survey of magnetism in massive stars: introduction and overview. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2-22, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2568. Acesso em: 24 jul. 2024.
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      Wade, G. A., Neiner, C., Alecian, E., & Carciofi, A. C. (2016). The MiMeS survey of magnetism in massive stars: introduction and overview. Monthly Notices of the Royal Astronomical Society, 456, 2-22. doi:10.1093/mnras/stv2568
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      Wade GA, Neiner C, Alecian E, Carciofi AC. The MiMeS survey of magnetism in massive stars: introduction and overview [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2-22.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stv2568
    • Vancouver

      Wade GA, Neiner C, Alecian E, Carciofi AC. The MiMeS survey of magnetism in massive stars: introduction and overview [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2-22.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stv2568
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH

    Assuntos: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS

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      NAKWACKI, Maria Soledad et al. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society, v. 455, n. 4, p. 3702-3723, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2586. Acesso em: 24 jul. 2024.
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      Nakwacki, M. S., Kowal, G., Santos-Lima, R., Dal Pino, E. M. de G., & Falceta Gonçalves, D. A. (2016). Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps. Monthly Notices of the Royal Astronomical Society, 455( 4), 3702-3723. doi:10.1093/mnras/stv2586
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      Nakwacki MS, Kowal G, Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455( 4): 3702-3723.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stv2586
    • Vancouver

      Nakwacki MS, Kowal G, Santos-Lima R, Dal Pino EM de G, Falceta Gonçalves DA. Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 455( 4): 3702-3723.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1093/mnras/stv2586
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: ASTROFÍSICA ESTELAR, CAMPO MAGNÉTICO

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      GUERRERO, G et al. On the role of tachoclines in solar and stellar dynamos. Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf. Acesso em: 24 jul. 2024.
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      Guerrero, G., Smolarkiewicz, P. K., Dal Pino, E. M. de G., Kosovichev, A. G., & Mansour, N. N. (2016). On the role of tachoclines in solar and stellar dynamos. Astrophysical Journal. doi:10.3847/0004-637X/819/2/104
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      Guerrero G, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. On the role of tachoclines in solar and stellar dynamos [Internet]. Astrophysical Journal. 2016 ;[citado 2024 jul. 24 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf
    • Vancouver

      Guerrero G, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. On the role of tachoclines in solar and stellar dynamos [Internet]. Astrophysical Journal. 2016 ;[citado 2024 jul. 24 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf
  • Fonte: Journal of Physics: Conference Series. Nome do evento: The Science of Ed Stone: Celebrating his 80th Birthday. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, MEIO INTERESTELAR

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      FRISCH, P C et al. Following the interstellar magnetic field from the heliosphere into space with polarized starlight. Journal of Physics: Conference Series. Bristol: Institute of Physics - IOP. Disponível em: http://iopscience.iop.org/article/10.1088/1742-6596/767/1/012010/pdf. Acesso em: 24 jul. 2024. , 2016
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      Frisch, P. C., Berdyugin, A. B., Pirola, V., Magalhães, A. M., Seriacopi, D. B., & Ferrari, T. (2016). Following the interstellar magnetic field from the heliosphere into space with polarized starlight. Journal of Physics: Conference Series. Bristol: Institute of Physics - IOP. doi:10.1088/1742-6596/767/1/012010
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      Frisch PC, Berdyugin AB, Pirola V, Magalhães AM, Seriacopi DB, Ferrari T. Following the interstellar magnetic field from the heliosphere into space with polarized starlight [Internet]. Journal of Physics: Conference Series. 2016 ;767 012010.[citado 2024 jul. 24 ] Available from: http://iopscience.iop.org/article/10.1088/1742-6596/767/1/012010/pdf
    • Vancouver

      Frisch PC, Berdyugin AB, Pirola V, Magalhães AM, Seriacopi DB, Ferrari T. Following the interstellar magnetic field from the heliosphere into space with polarized starlight [Internet]. Journal of Physics: Conference Series. 2016 ;767 012010.[citado 2024 jul. 24 ] Available from: http://iopscience.iop.org/article/10.1088/1742-6596/767/1/012010/pdf
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIAS, MEIO INTERESTELAR, NUVENS DE MAGALHÃES, CAMPO MAGNÉTICO

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      GOMES, Aiara Lobo et al. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure. The Astrophysical Journal, v. 806, p. 94/1-94/19, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/806/1/94. Acesso em: 24 jul. 2024.
    • APA

      Gomes, A. L., Magalhães, A. M., Pereyra, A., & Rodrigues, C. V. (2015). A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure. The Astrophysical Journal, 806, 94/1-94/19. doi:10.1088/0004-637X/806/1/94
    • NLM

      Gomes AL, Magalhães AM, Pereyra A, Rodrigues CV. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure [Internet]. The Astrophysical Journal. 2015 ; 806 94/1-94/19.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
    • Vancouver

      Gomes AL, Magalhães AM, Pereyra A, Rodrigues CV. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure [Internet]. The Astrophysical Journal. 2015 ; 806 94/1-94/19.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: POEIRA INTERESTELAR, MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), SOL

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      FRISCH, P. C et al. Evidence for an interstellar dust filament in the outer heliosheath. The Astrophysical Journal, v. 805, p. 60/1-60/8, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/805/1/60. Acesso em: 24 jul. 2024.
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      Frisch, P. C., Andersson, B. -G., Berdyugin, A., Piirola, V., Funsten, H. O., Magalhães, A. M., et al. (2015). Evidence for an interstellar dust filament in the outer heliosheath. The Astrophysical Journal, 805, 60/1-60/8. doi:10.1088/0004-637X/805/1/60
    • NLM

      Frisch PC, Andersson B-G, Berdyugin A, Piirola V, Funsten HO, Magalhães AM, Seriacopi DB, McComas DJ, Schwadron NA, Slavin JD, Wiktorowicz SJ. Evidence for an interstellar dust filament in the outer heliosheath [Internet]. The Astrophysical Journal. 2015 ; 805 60/1-60/8.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/0004-637X/805/1/60
    • Vancouver

      Frisch PC, Andersson B-G, Berdyugin A, Piirola V, Funsten HO, Magalhães AM, Seriacopi DB, McComas DJ, Schwadron NA, Slavin JD, Wiktorowicz SJ. Evidence for an interstellar dust filament in the outer heliosheath [Internet]. The Astrophysical Journal. 2015 ; 805 60/1-60/8.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/0004-637X/805/1/60
  • Fonte: JournalofPhysics: Conference Series. Nome do evento: Annual International Astrophysics Conference: Voyager, IBEX, and the Interstellar Medium. Unidade: IAG

    Assuntos: MEIO INTERESTELAR, CAMPO MAGNÉTICO

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    • ABNT

      FRISCH, P. C et al. Connecting the interstellar magnetic field at the heliosphere to the Loop I superbubble. JournalofPhysics: Conference Series. Bristol: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Disponível em: https://doi.org/10.1088/1742-6596/577/1/012010. Acesso em: 24 jul. 2024. , 2015
    • APA

      Frisch, P. C., Berdyugin, A., Funsten, H. O., Magalhães, A. M., McComas, D. J., Piirola, V., et al. (2015). Connecting the interstellar magnetic field at the heliosphere to the Loop I superbubble. JournalofPhysics: Conference Series. Bristol: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. doi:10.1088/1742-6596/577/1/012010
    • NLM

      Frisch PC, Berdyugin A, Funsten HO, Magalhães AM, McComas DJ, Piirola V, Schwadron NA, Seriacopi DB, Wiktorowicz SJ. Connecting the interstellar magnetic field at the heliosphere to the Loop I superbubble [Internet]. JournalofPhysics: Conference Series. 2015 ; 577 012010/1-012010/10.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/1742-6596/577/1/012010
    • Vancouver

      Frisch PC, Berdyugin A, Funsten HO, Magalhães AM, McComas DJ, Piirola V, Schwadron NA, Seriacopi DB, Wiktorowicz SJ. Connecting the interstellar magnetic field at the heliosphere to the Loop I superbubble [Internet]. JournalofPhysics: Conference Series. 2015 ; 577 012010/1-012010/10.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1088/1742-6596/577/1/012010
  • Fonte: Astronomische Nachrichten. Unidade: IAG

    Assuntos: CAMPO MAGNÉTICO, PULSARES, QUARK

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      MANREZA PARET, D e HORVATH, Jorge Ernesto e PEREZ MARTÍNEZ, A. Anisotropic structure equations in magnetized quark stars. Astronomische Nachrichten, v. 336, n. 8/9, p. 856-860, 2015Tradução . . Disponível em: https://doi.org/10.1002/asna.201512237. Acesso em: 24 jul. 2024.
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      Manreza Paret, D., Horvath, J. E., & Perez Martínez, A. (2015). Anisotropic structure equations in magnetized quark stars. Astronomische Nachrichten, 336( 8/9), 856-860. doi:10.1002/asna.201512237
    • NLM

      Manreza Paret D, Horvath JE, Perez Martínez A. Anisotropic structure equations in magnetized quark stars [Internet]. Astronomische Nachrichten. 2015 ; 336( 8/9): 856-860.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1002/asna.201512237
    • Vancouver

      Manreza Paret D, Horvath JE, Perez Martínez A. Anisotropic structure equations in magnetized quark stars [Internet]. Astronomische Nachrichten. 2015 ; 336( 8/9): 856-860.[citado 2024 jul. 24 ] Available from: https://doi.org/10.1002/asna.201512237

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