ReP USP - Resultado da busca

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, D; Lazarian, A; Nakwacki, M. S
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: AGLOMERADOS DE GALÁXIAS, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, TURBULÊNCIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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. 84, p. 1-21, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/781/2/84. Acesso em: 03 out. 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 out. 03 ] 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 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 03 out. 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 out. 03 ] 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 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
Artigo de periodico
The collapse of turbulent cores and reconnection diffusion (2013)
Leão, M. R. M; Dal Pino, Elisabete Maria de Gouveia; Santos-Lima, R; Lazarian, A
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, FORMAÇÃO DE ESTRELAS, TURBULÊNCIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LEÃO, M. R. M et al. The collapse of turbulent cores and reconnection diffusion. The Astrophysical Journal, v. 777, n. 1, p. 46/1-46/23, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/777/1/46. Acesso em: 03 out. 2024.
APA
Leão, M. R. M., Dal Pino, E. M. de G., Santos-Lima, R., & Lazarian, A. (2013). The collapse of turbulent cores and reconnection diffusion. The Astrophysical Journal, 777( 1), 46/1-46/23. doi:10.1088/0004-637X/777/1/46
NLM
Leão MRM, Dal Pino EM de G, Santos-Lima R, Lazarian A. The collapse of turbulent cores and reconnection diffusion [Internet]. The Astrophysical Journal. 2013 ; 777( 1): 46/1-46/23.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/777/1/46
Vancouver
Leão MRM, Dal Pino EM de G, Santos-Lima R, Lazarian A. The collapse of turbulent cores and reconnection diffusion [Internet]. The Astrophysical Journal. 2013 ; 777( 1): 46/1-46/23.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/777/1/46
Artigo de periodico
The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks (2012)
Santos-Lima, R; Dal Pino, Elisabete Maria de Gouveia; Lazarian, A
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, MEIO INTERESTELAR, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, FORMAÇÃO DE ESTRELAS, TURBULÊNCIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS-LIMA, R e DAL PINO, Elisabete Maria de Gouveia e LAZARIAN, A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks. The Astrophysical Journal, v. 747, p. 21/1-21/8, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/747/1/21. Acesso em: 03 out. 2024.
APA
Santos-Lima, R., Dal Pino, E. M. de G., & Lazarian, A. (2012). The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks. The Astrophysical Journal, 747, 21/1-21/8. doi:10.1088/0004-637X/747/1/21
NLM
Santos-Lima R, Dal Pino EM de G, Lazarian A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks [Internet]. The Astrophysical Journal. 2012 ; 747 21/1-21/8.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21
Vancouver
Santos-Lima R, Dal Pino EM de G, Lazarian A. The role of turbulent magnetic reconnection in the formation of rotationally supported protostellar disks [Internet]. The Astrophysical Journal. 2012 ; 747 21/1-21/8.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/747/1/21
Artigo de periodico
Evolution and lifetime of transient clumps in the turbulent interstellar medium (2011)
Falceta Gonçalves, Diego Antonio; Lazarian, A
Source: The Astrophysical Journal. Unidade: EACH
Assunto: ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
FALCETA GONÇALVES, Diego Antonio e LAZARIAN, A. Evolution and lifetime of transient clumps in the turbulent interstellar medium. The Astrophysical Journal, v. 735, n. 2, p. 1-7, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/735/2/99. Acesso em: 03 out. 2024.
APA
Falceta Gonçalves, D. A., & Lazarian, A. (2011). Evolution and lifetime of transient clumps in the turbulent interstellar medium. The Astrophysical Journal, 735( 2), 1-7. doi:10.1088/0004-637X/735/2/99
NLM
Falceta Gonçalves DA, Lazarian A. Evolution and lifetime of transient clumps in the turbulent interstellar medium [Internet]. The Astrophysical Journal. 2011 ; 735( 2): 1-7.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99
Vancouver
Falceta Gonçalves DA, Lazarian A. Evolution and lifetime of transient clumps in the turbulent interstellar medium [Internet]. The Astrophysical Journal. 2011 ; 735( 2): 1-7.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99
Artigo de periodico
Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection (2010)
Santos-Lima, R; Lazarian, A; Dal Pino, Elisabete Maria de Gouveia; Cho, J
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, FORMAÇÃO DE ESTRELAS, TURBULÊNCIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS-LIMA, R et al. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal, v. 714, p. 442\2013461, 2010Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/714/1/442. Acesso em: 03 out. 2024.
APA
Santos-Lima, R., Lazarian, A., Dal Pino, E. M. de G., & Cho, J. (2010). Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal, 714, 442\2013461. doi:10.1088/0004-637X/714/1/442
NLM
Santos-Lima R, Lazarian A, Dal Pino EM de G, Cho J. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection [Internet]. The Astrophysical Journal. 2010 ; 714 442\2013461.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/714/1/442
Vancouver
Santos-Lima R, Lazarian A, Dal Pino EM de G, Cho J. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection [Internet]. The Astrophysical Journal. 2010 ; 714 442\2013461.[citado 2024 out. 03 ] Available from: https://doi.org/10.1088/0004-637X/714/1/442
Artigo de periodico
Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection (2010)
Santos-Lima, R; Lazarian, A; Gouveia dal Pino, Elisabete Maria de; Cho, J.
Source: The Astrophysical Journal. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, FORMAÇÃO DE ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS-LIMA, R et al. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal, v. 714, p. 442-461, 2010Tradução . . Acesso em: 03 out. 2024.
APA
Santos-Lima, R., Lazarian, A., Gouveia dal Pino, E. M. de, & Cho, J. (2010). Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal, 714, 442-461.
NLM
Santos-Lima R, Lazarian A, Gouveia dal Pino EM de, Cho J. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal. 2010 ; 714 442-461.[citado 2024 out. 03 ]
Vancouver
Santos-Lima R, Lazarian A, Gouveia dal Pino EM de, Cho J. Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection. The Astrophysical Journal. 2010 ; 714 442-461.[citado 2024 out. 03 ]
Artigo de periodico
Constraints on the acceleration of ultra-high-energy cosmic rays in accretion-induced collapse pulsars (2001)
Gouveia dal Pino, Elisabete Maria de; Lazarian, A
Source: The Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GOUVEIA DAL PINO, Elisabete Maria de e LAZARIAN, A. Constraints on the acceleration of ultra-high-energy cosmic rays in accretion-induced collapse pulsars. The Astrophysical Journal, v. 560, p. 358-364, 2001Tradução . . Acesso em: 03 out. 2024.
APA
Gouveia dal Pino, E. M. de, & Lazarian, A. (2001). Constraints on the acceleration of ultra-high-energy cosmic rays in accretion-induced collapse pulsars. The Astrophysical Journal, 560, 358-364.
NLM
Gouveia dal Pino EM de, Lazarian A. Constraints on the acceleration of ultra-high-energy cosmic rays in accretion-induced collapse pulsars. The Astrophysical Journal. 2001 ; 560 358-364.[citado 2024 out. 03 ]
Vancouver
Gouveia dal Pino EM de, Lazarian A. Constraints on the acceleration of ultra-high-energy cosmic rays in accretion-induced collapse pulsars. The Astrophysical Journal. 2001 ; 560 358-364.[citado 2024 out. 03 ]

USP Schools

ReP

Filtros

Authors

Date published

Subjects

Non normalized affiliation