ReP USP - Resultado da busca

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
Fonte: The Astrophysical Journal. Unidade: EACH
Assuntos: 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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
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
Fonte: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Assuntos: 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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] 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
Fonte: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, EACH
Assuntos: CAMPO MAGNÉTICO, TURBULÊNCIA, GALÁXIAS
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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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] 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
Fonte: IAU Highlights of Astronomy, v. 16. Nome do evento: IAU General Assembly. Unidades: IAG, EACH
Assuntos: 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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] Available from: https://doi.org/10.1017/S1743921314011740
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
Fonte: The Astrophysical Journal. Unidade: EACH
Assuntos: 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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
Artigo de periodico
On the alignment of PNe and local magnetic field at the Galactic centre: magnetohydrodynamical numerical simulations (2014)
Falceta Gonçalves, Diego Antonio; Monteiro, H
Fonte: Monthly notices of the Royal Astronomical Society. Unidade: EACH
Assuntos: GALÁXIAS, CAMPO MAGNÉTICO, NEBULOSAS, MAGNETOHIDRODINÂMICA
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ABNT
FALCETA GONÇALVES, Diego Antonio e MONTEIRO, H. On the alignment of PNe and local magnetic field at the Galactic centre: magnetohydrodynamical numerical simulations. Monthly notices of the Royal Astronomical Society, v. 438, n. 4, p. 2853-2863, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt2393. Acesso em: 04 ago. 2024.
APA
Falceta Gonçalves, D. A., & Monteiro, H. (2014). On the alignment of PNe and local magnetic field at the Galactic centre: magnetohydrodynamical numerical simulations. Monthly notices of the Royal Astronomical Society, 438( 4), 2853-2863. doi:10.1093/mnras/stt2393
NLM
Falceta Gonçalves DA, Monteiro H. On the alignment of PNe and local magnetic field at the Galactic centre: magnetohydrodynamical numerical simulations [Internet]. Monthly notices of the Royal Astronomical Society. 2014 ; 438( 4): 2853-2863.[citado 2024 ago. 04 ] Available from: https://doi.org/10.1093/mnras/stt2393
Vancouver
Falceta Gonçalves DA, Monteiro H. On the alignment of PNe and local magnetic field at the Galactic centre: magnetohydrodynamical numerical simulations [Internet]. Monthly notices of the Royal Astronomical Society. 2014 ; 438( 4): 2853-2863.[citado 2024 ago. 04 ] Available from: https://doi.org/10.1093/mnras/stt2393
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
Fonte: The Astrophysical Journal. Unidades: IAG, EACH
Assuntos: 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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
Artigo de periodico
The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts (2013)
Ruiz, L. O; Falceta Gonçalves, Diego Antonio; Lanfranchi, Gustavo Amaral; Caproni, Anderson
Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: EACH
Assuntos: GALÁXIAS, ESTRELAS, MATÉRIA ESCURA, EVOLUÇÃO ESTELAR
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ABNT
RUIZ, L. O et al. The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts. Monthly Notices of the Royal Astronomical Society, v. 429, n. 2, p. 1437\20131449, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/sts425. Acesso em: 04 ago. 2024.
APA
Ruiz, L. O., Falceta Gonçalves, D. A., Lanfranchi, G. A., & Caproni, A. (2013). The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts. Monthly Notices of the Royal Astronomical Society, 429( 2), 1437\20131449. doi:10.1093/mnras/sts425
NLM
Ruiz LO, Falceta Gonçalves DA, Lanfranchi GA, Caproni A. The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429( 2): 1437\20131449.[citado 2024 ago. 04 ] Available from: https://doi.org/10.1093/mnras/sts425
Vancouver
Ruiz LO, Falceta Gonçalves DA, Lanfranchi GA, Caproni A. The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 429( 2): 1437\20131449.[citado 2024 ago. 04 ] Available from: https://doi.org/10.1093/mnras/sts425
Artigo de periodico
On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds (2013)
Falceta Gonçalves, Diego Antonio
Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: EACH
Assuntos: GALÁXIAS, JATOS (ASTRONOMIA), MEIO INTERGALÁTICO, MATÉRIA ESCURA
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ABNT
FALCETA GONÇALVES, Diego Antonio. On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds. Monthly Notices of the Royal Astronomical Society, v. 432, n. ju 2013, p. 589\2013597, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt485. Acesso em: 04 ago. 2024.
APA
Falceta Gonçalves, D. A. (2013). On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds. Monthly Notices of the Royal Astronomical Society, 432( ju 2013), 589\2013597. doi:10.1093/mnras/stt485
NLM
Falceta Gonçalves DA. On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 432( ju 2013): 589\2013597.[citado 2024 ago. 04 ] Available from: https://doi.org/10.1093/mnras/stt485
Vancouver
Falceta Gonçalves DA. On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 432( ju 2013): 589\2013597.[citado 2024 ago. 04 ] Available from: https://doi.org/10.1093/mnras/stt485
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
Fonte: Jets at all scales: Proceedings. Nome do evento: IAU Symposium. Unidades: IAG, EACH
Assuntos: 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: 04 ago. 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 ago. 04 ] 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 ago. 04 ] 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
Fonte: The Astronomical Journal. Unidades: EACH, IAG
Assuntos: 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: 04 ago. 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 ago. 04 ]
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 ago. 04 ]

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