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Artigo de periodico
Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback (2017)
Santos-Lima, Reinaldo; Dal Pino, Elisabete Maria de Gouveia; Falceta Gonçalves, Diego Antonio; Nakwacki, Maria Soledad; Kowal, Grzegorz
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Subjects: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS, MEIO INTERESTELAR
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ABNT
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: 08 set. 2024.
APA
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 set. 08 ] 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 set. 08 ] Available from: https://doi.org/10.1093/mnras/stw3050
Artigo de periodico
Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps (2016)
Nakwacki, Maria Soledad; Kowal, Grzegorz; Santos-Lima, Reinaldo; Dal Pino, Elisabete Maria de Gouveia; Falceta Gonçalves, Diego Antonio
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Subjects: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 08 set. 2024.
APA
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
NLM
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 set. 08 ] 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 set. 08 ] Available from: https://doi.org/10.1093/mnras/stv2586
Trabalho de evento
MHD turbulence in the intracluster medium (2015)
Falceta Gonçalves, Diego Antonio; Kowal, G.; Dal Pino, Elisabete Maria de Gouveia; Santos-Lima, R; Nakwacki, S; Lazarian, A
Source: IAU Highlights of Astronomy, v. 16. Conference titles: IAU General Assembly. Unidades: IAG, EACH
Subjects: GALÁXIAS, AGLOMERADOS DE GALÁXIAS, MEIO INTERGALÁTICO, CAMPO MAGNÉTICO
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ABNT
FALCETA GONÇALVES, Diego Antonio et al. MHD turbulence in the intracluster medium. 2015, Anais.. Cambridge: Cambridge University Press, 2015. Disponível em: https://doi.org/10.1017/S1743921314011740. Acesso em: 08 set. 2024.
APA
Falceta Gonçalves, D. A., Kowal, G., Dal Pino, E. M. de G., Santos-Lima, R., Nakwacki, S., & Lazarian, A. (2015). MHD turbulence in the intracluster medium. In IAU Highlights of Astronomy, v. 16. Cambridge: Cambridge University Press. doi:10.1017/S1743921314011740
NLM
Falceta Gonçalves DA, Kowal G, Dal Pino EM de G, Santos-Lima R, Nakwacki S, Lazarian A. MHD turbulence in the intracluster medium [Internet]. IAU Highlights of Astronomy, v. 16. 2015 ;[citado 2024 set. 08 ] Available from: https://doi.org/10.1017/S1743921314011740
Vancouver
Falceta Gonçalves DA, Kowal G, Dal Pino EM de G, Santos-Lima R, Nakwacki S, Lazarian A. MHD turbulence in the intracluster medium [Internet]. IAU Highlights of Astronomy, v. 16. 2015 ;[citado 2024 set. 08 ] Available from: https://doi.org/10.1017/S1743921314011740
Artigo de periodico
Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium (2014)
Santos-Lima, R; Dal Pino, Elisabete Maria de Gouveia; Kowal, G; Falceta Gonçalves, Diego Antonio; Lazarian, A; Nakwacki, M. S
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: 08 set. 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 set. 08 ] 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 set. 08 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
Trabalho de evento
The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275) (2011)
Teixeira, D. M.; Abraham, Zulema; Caproni, A; Falceta Gonçalves, Diego Antonio
Source: Jets at all scales: Proceedings. Conference titles: IAU Symposium. Unidades: IAG, EACH
Subjects: GALÁXIAS, JATOS (ASTRONOMIA), DISCOS DE ACRESÇÂO
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ABNT
TEIXEIRA, D. M. et al. The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275). 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921310015954. Acesso em: 08 set. 2024.
APA
Teixeira, D. M., Abraham, Z., Caproni, A., & Falceta Gonçalves, D. A. (2011). The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275). In Jets at all scales: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921310015954
NLM
Teixeira DM, Abraham Z, Caproni A, Falceta Gonçalves DA. The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275) [Internet]. Jets at all scales: Proceedings. 2011 ;[citado 2024 set. 08 ] Available from: https://doi.org/10.1017/S1743921310015954
Vancouver
Teixeira DM, Abraham Z, Caproni A, Falceta Gonçalves DA. The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275) [Internet]. Jets at all scales: Proceedings. 2011 ;[citado 2024 set. 08 ] Available from: https://doi.org/10.1017/S1743921310015954
Artigo de periodico
A survey of Early-Type Stars based on the two micron all sky survey database (2007)
Ortiz, R.; Malacarne, M; Wilhelm, R; Costa, R D D; Rossi, S; Maciel, Walter Junqueira; Costa, A. F. M
Source: The Astronomical Journal. Unidades: EACH, IAG
Subjects: GALÁXIAS, ESTRELAS
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ABNT
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: 08 set. 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 set. 08 ]
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 set. 08 ]

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