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Artigo de periodico
Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? (2020)
Kowal, Grzegorz ; Falceta Gonçalves, Diego Antonio ; Lazarian, Alex ; Vishniac, Ethan T
Source: The Astrophysical Journal. Unidade: EACH
Subjects: TURBULÊNCIA, ASTROFÍSICA
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ABNT
KOWAL, Grzegorz et al. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?. The Astrophysical Journal, v. 892, n. 1, p. 01-15, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab7a13. Acesso em: 05 nov. 2024.
APA
Kowal, G., Falceta Gonçalves, D. A., Lazarian, A., & Vishniac, E. T. (2020). Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? The Astrophysical Journal, 892( 1), 01-15. doi:10.3847/1538-4357/ab7a13
NLM
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? [Internet]. The Astrophysical Journal. 2020 ; 892( 1): 01-15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
Vancouver
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? [Internet]. The Astrophysical Journal. 2020 ; 892( 1): 01-15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
Artigo de periodico
Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium (2020)
Jesus, Lorena do Carmo ; González-Casanova, Diego F. ; Falceta Gonçalves, Diego Antonio ; Lazarian, Alex ; Jablonski, Francisco; Zhang, Jian-Fu; Ferreira, Ivan Soares ; Castro, Manuel L. Díaz; Yang, Bo
Source: The Astrophysical Journal. Unidade: EACH
Subjects: MAGNETOHIDRODINÂMICA, MEIO INTERESTELAR
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ABNT
JESUS, Lorena do Carmo et al. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, v. 905, n. 2, p. 01-12, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abc331. Acesso em: 05 nov. 2024.
APA
Jesus, L. do C., González-Casanova, D. F., Falceta Gonçalves, D. A., Lazarian, A., Jablonski, F., Zhang, J. -F., et al. (2020). Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, 905( 2), 01-12. doi:10.3847/1538-4357/abc331
NLM
Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/abc331
Vancouver
Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/abc331
Artigo de periodico
Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models (2017)
Caproni, Anderson; Lanfranchi, Gustavo Amaral; Baio, Gabriel Henrique Campos; Kowal, Grzegorz; Falceta Gonçalves, Diego Antonio
Source: The Astrophysical Journal. Unidade: EACH
Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR, MAGNETOHIDRODINÂMICA
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ABNT
CAPRONI, Anderson et al. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, v. 838, n. 2, p. 1-9, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6002. Acesso em: 05 nov. 2024.
APA
Caproni, A., Lanfranchi, G. A., Baio, G. H. C., Kowal, G., & Falceta Gonçalves, D. A. (2017). Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, 838( 2), 1-9. doi:10.3847/1538-4357/aa6002
NLM
Caproni A, Lanfranchi GA, Baio GHC, Kowal G, Falceta Gonçalves DA. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
Vancouver
Caproni A, Lanfranchi GA, Baio GHC, Kowal G, Falceta Gonçalves DA. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
Artigo de periodico
Statistics of reconnection-driven turbulence (2017)
Kowal, Grzegorz; Falceta Gonçalves, Diego Antonio; Lazarian, Alex; Vishniac, Ethan T.
Source: The Astrophysical Journal. Unidade: EACH
Subjects: TURBULÊNCIA, MAGNETOHIDRODINÂMICA
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ABNT
KOWAL, Grzegorz et al. Statistics of reconnection-driven turbulence. The Astrophysical Journal, v. 838, n. 2, p. 1-13, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6001. Acesso em: 05 nov. 2024.
APA
Kowal, G., Falceta Gonçalves, D. A., Lazarian, A., & Vishniac, E. T. (2017). Statistics of reconnection-driven turbulence. The Astrophysical Journal, 838( 2), 1-13. doi:10.3847/1538-4357/aa6001
NLM
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aa6001
Vancouver
Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aa6001
Artigo de periodico
Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media (2015)
Falceta Gonçalves, Diego Antonio; Kowal, Grzegorz
Source: The Astrophysical Journal. Unidade: EACH
Subjects: MEIO INTERGALÁTICO, CAMPO MAGNÉTICO, TURBULÊNCIA, UNIVERSO PRIMORDIAL
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ABNT
FALCETA GONÇALVES, Diego Antonio e KOWAL, Grzegorz. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media. The Astrophysical Journal, v. 808, n. 1, p. 1-15, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/65. Acesso em: 05 nov. 2024.
APA
Falceta Gonçalves, D. A., & Kowal, G. (2015). Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media. The Astrophysical Journal, 808( 1), 1-15. doi:10.1088/0004-637X/808/1/65
NLM
Falceta Gonçalves DA, Kowal G. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media [Internet]. The Astrophysical Journal. 2015 ; 808( 1): 1-15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/808/1/65
Vancouver
Falceta Gonçalves DA, Kowal G. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media [Internet]. The Astrophysical Journal. 2015 ; 808( 1): 1-15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/808/1/65
Artigo de periodico
Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor (2015)
Caproni, Anderson; Lanfranchi, Gustavo Amaral; Silva, A. Luiz da; Falceta Gonçalves, Diego Antonio
Source: The Astrophysical Journal. Unidade: EACH
Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR, HIDRODINÂMICA
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ABNT
CAPRONI, Anderson et al. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, v. 805, n. ju 2015, p. 1-12, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/805/2/109. Acesso em: 05 nov. 2024.
APA
Caproni, A., Lanfranchi, G. A., Silva, A. L. da, & Falceta Gonçalves, D. A. (2015). Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, 805( ju 2015), 1-12. doi:10.1088/0004-637X/805/2/109
NLM
Caproni A, Lanfranchi GA, Silva AL da, Falceta Gonçalves DA. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
Vancouver
Caproni A, Lanfranchi GA, Silva AL da, Falceta Gonçalves DA. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
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: 05 nov. 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 nov. 05 ] 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 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
Artigo de periodico
η Carinae baby homunculus uncovered by ALMA (2014)
Abraham, Zulema; Falceta Gonçalves, Diego Antonio; Beaklini, Pedro Paulo Bonetti
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: ESTRELAS BINÁRIAS, PERDA DE MASSA, VENTO, ASTROFÍSICA ESTELAR
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ABNT
ABRAHAM, Zulema e FALCETA GONÇALVES, Diego Antonio e BEAKLINI, Pedro Paulo Bonetti. η Carinae baby homunculus uncovered by ALMA. The Astrophysical Journal, v. 791, n. 2, p. 1-10, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/791/2/95. Acesso em: 05 nov. 2024.
APA
Abraham, Z., Falceta Gonçalves, D. A., & Beaklini, P. P. B. (2014). η Carinae baby homunculus uncovered by ALMA. The Astrophysical Journal, 791( 2), 1-10. doi:10.1088/0004-637X/791/2/95
NLM
Abraham Z, Falceta Gonçalves DA, Beaklini PPB. η Carinae baby homunculus uncovered by ALMA [Internet]. The Astrophysical Journal. 2014 ; 791( 2): 1-10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/791/2/95
Vancouver
Abraham Z, Falceta Gonçalves DA, Beaklini PPB. η Carinae baby homunculus uncovered by ALMA [Internet]. The Astrophysical Journal. 2014 ; 791( 2): 1-10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/791/2/95
Artigo de periodico
Magnetic field components analysis of the SCUPOL 850 'mü'm polarization data catalog (2013)
Poidevin, Frédérick; Falceta Gonçalves, Diego Antonio; Kowal, Grzegorz; Dal Pino, Elisabete Maria de Gouveia; Magalhães, Antonio Mário
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), TURBULÊNCIA
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ABNT
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: 05 nov. 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 nov. 05 ] 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 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/777/2/112
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
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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: 05 nov. 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 nov. 05 ] 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 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99
Artigo de periodico
Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 (2011)
Monteiro, Hektor; Falceta Gonçalves, Diego Antonio
Source: The Astrophysical Journal. Unidade: EACH
Subjects: ASTROFÍSICA ESTELAR, NEBULOSAS, MEIO INTERGALÁTICO
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ABNT
MONTEIRO, Hektor e FALCETA GONÇALVES, Diego Antonio. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40. The Astrophysical Journal, v. 738, n. 2, p. 1-10, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/738/2/174. Acesso em: 05 nov. 2024.
APA
Monteiro, H., & Falceta Gonçalves, D. A. (2011). Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40. The Astrophysical Journal, 738( 2), 1-10. doi:10.1088/0004-637X/738/2/174
NLM
Monteiro H, Falceta Gonçalves DA. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 [Internet]. The Astrophysical Journal. 2011 ; 738( 2): 1-10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/738/2/174
Vancouver
Monteiro H, Falceta Gonçalves DA. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 [Internet]. The Astrophysical Journal. 2011 ; 738( 2): 1-10.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1088/0004-637X/738/2/174

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