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Artigo de periodico
Whence the interstellar magnetic field shaping the heliosphere? (2022)
Frisch, P. C ; Piirola, V. ; Magalhães, Antonio Mário
Source: Astrophysical Journal Supplement Series. Unidade: IAG
Subjects: 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: 18 nov. 2024.
APA
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
NLM
Frisch PC, Piirola V, Magalhães AM. Whence the interstellar magnetic field shaping the heliosphere? [Internet]. Astrophysical Journal Supplement Series. 2022 ; 259 48.[citado 2024 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/ac5750
Artigo de periodico
Diffusion of large-scale magnetic fields by reconnection in MHD turbulence (2021)
Santos-Lima, R ; Guerrero, G; Dal Pino, Elisabete Maria de Gouveia ; Lazarian, A.
Source: 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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: https://academic.oup.com/mnras/article/503/1/1290/6144594
Artigo de periodico
Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA (2019)
Leaman, Ryan; Coelho, Paula Rodrigues Teixeira
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: 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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz1844
Artigo de periodico
Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration (2019)
Páez, A.; Jatenco-Pereira, Vera ; Gonçalves, Diego Antonio Falceta ; Opher, M.
Source: The Astrophysical Journal. Unidades: IAG, EACH
Subjects: 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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
Vancouver
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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
Artigo de periodico
The impact of plasma instabilities on the spectra of TeV blazars (2019)
Batista, Rafael Alves; Saveliev, Andrey; Dal Pino, Elisabete Maria de Gouveia
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: 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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz2389
Vancouver
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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz2389
Artigo de periodico
What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? (2019)
Guerrero, G; Zaire, B; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia ; Kosovichev, A. G; Mansour, N. N
Source: The Astrophysical Journal. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR
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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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
Artigo de periodico
Magnetic field decay in black widow pulsars (2018)
Mendes, Camile; Avellar, Marcio G. B. de; Horvath, Jorge Ernesto; Souza, Rodrigo A. de; Benvenuto, O G; De Vito, M. A
Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG
Subjects: 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: 18 nov. 2024.
APA
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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stx3319
Vancouver
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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stx3319
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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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stw3050
Artigo de periodico
Kelvin–Helmholtz instability at the CME–Sheath and Sheath–Solar-wind interfaces (2017)
Murcia, Miguel Andres Paez; Pereira, Vera Jatenco Silva; Gonçalves, Diego Antonio Falceta; opher, merav
Source: The Astrophysical Journal: an international review of astronomy and astronomical physics. Unidades: EACH, IAG
Subjects: 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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/aa9753
Trabalho de evento
HD151018: strong magnetic field in a giant O-type star? (2017)
Rubinho, Marcelo Soares; Damineli Neto, Augusto; Carciofi, Alex Cavaliéri; Moser, D
Source: 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. Conference titles: IAU SYMPOSIUM. Unidade: IAG
Subjects: 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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003477
Artigo de periodico
Understanding solar torsional oscillations from global dynamo models (2016)
Guerrero, G; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia
Source: Astrophysical Journal Letters. Unidade: IAG
Subjects: 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: 18 nov. 2024.
APA
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
NLM
Guerrero G, Smolarkiewicz PK, Dal Pino EM de G. Understanding solar torsional oscillations from global dynamo models [Internet]. Astrophysical Journal Letters. 2016 ;[citado 2024 nov. 18 ] 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 nov. 18 ] Available from: https://arxiv.org/abs/1608.02278
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
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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stv2586
Artigo de periodico
On the role of tachoclines in solar and stellar dynamos (2016)
Guerrero, G; Smolarkiewicz, P. K; Dal Pino, Elisabete Maria de Gouveia; Kosovichev, A. G; Mansour, N. N
Source: Astrophysical Journal. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, CAMPO MAGNÉTICO
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ABNT
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: 18 nov. 2024.
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/819/2/104/pdf
Trabalho de evento-anais periodico
Following the interstellar magnetic field from the heliosphere into space with polarized starlight (2016)
Frisch, P C; Berdyugin, A B; Pirola, V; Magalhães, Antonio Mário; Seriacopi, D B; Ferrari, T
Source: Journal of Physics: Conference Series. Conference titles: The Science of Ed Stone: Celebrating his 80th Birthday. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, MEIO INTERESTELAR
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ABNT
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: 18 nov. 2024. , 2016
APA
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
NLM
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 nov. 18 ] 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 nov. 18 ] Available from: http://iopscience.iop.org/article/10.1088/1742-6596/767/1/012010/pdf
Artigo de periodico
A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure (2015)
Gomes, Aiara Lobo; Magalhães, Antônio Mário; Pereyra, Antonio; Rodrigues, Cláudia Vilega
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS, MEIO INTERESTELAR, NUVENS DE MAGALHÃES, CAMPO MAGNÉTICO
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ABNT
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
Artigo de periodico
Evidence for an interstellar dust filament in the outer heliosheath (2015)
Frisch, P. C; Andersson, B.-G; Berdyugin, A; Piirola, V; Funsten, H. O; Magalhães, Antonio Mário; Seriacopi, D. B; McComas, D. J; Schwadron, N. A; Slavin, J. D; Wiktorowicz, S. J
Source: The Astrophysical Journal. Unidade: IAG
Subjects: POEIRA INTERESTELAR, MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), SOL
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 18 nov. 2024.
APA
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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1088/0004-637X/805/1/60
Trabalho de evento-anais periodico
Connecting the interstellar magnetic field at the heliosphere to the Loop I superbubble (2015)
Frisch, P. C; Berdyugin, A; Funsten, H. O; Magalhães, Antonio Mário; McComas, D. J; Piirola, V; Schwadron, N. A; Seriacopi, D. B; Wiktorowicz, S. J
Source: JournalofPhysics: Conference Series. Conference titles: Annual International Astrophysics Conference: Voyager, IBEX, and the Interstellar Medium. Unidade: IAG
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1088/1742-6596/577/1/012010
Artigo de periodico
Anisotropic structure equations in magnetized quark stars (2015)
Manreza Paret, D; Horvath, Jorge Ernesto; Perez Martínez, A
Source: Astronomische Nachrichten. Unidade: IAG
Subjects: CAMPO MAGNÉTICO, PULSARES, QUARK
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 18 nov. 2024.
APA
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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1002/asna.201512237
Artigo de periodico
Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible (2015)
Ade, P. A. R; Aghanim, N; Magalhães, Antonio Mário
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: POLARIZAÇÃO (ASTRONOMIA), POEIRA INTERESTELAR, NUVENS, MEIO INTERESTELAR, CAMPO MAGNÉTICO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ADE, P. A. R e AGHANIM, N e MAGALHÃES, Antonio Mário. Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible. Astronomy & Astrophysics, v. 576, p. A106/1-A106/4, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424087. Acesso em: 18 nov. 2024.
APA
Ade, P. A. R., Aghanim, N., & Magalhães, A. M. (2015). Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible. Astronomy & Astrophysics, 576, A106/1-A106/4. doi:10.1051/0004-6361/201424087
NLM
Ade PAR, Aghanim N, Magalhães AM. Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible [Internet]. Astronomy & Astrophysics. 2015 ; 576 A106/1-A106/4.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201424087
Vancouver
Ade PAR, Aghanim N, Magalhães AM. Planck intermediate results: XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible [Internet]. Astronomy & Astrophysics. 2015 ; 576 A106/1-A106/4.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201424087
Trabalho de evento
Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog (2015)
Poidevin, Frédérick; Falceta-Gonçalves, Diego; Kowal, Grzegorz; Dal Pino, Elisabete Maria de Gouveia; Magalhães, Antonio Mário
Source: IAU Highlights of Astronomy, v. 16. Conference titles: IAU General Assembly. Unidade: IAG
Subjects: MEIO INTERESTELAR, CAMPO MAGNÉTICO, NUVENS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
POIDEVIN, Frédérick et al. Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog. 2015, Anais.. Cambridge: Cambridge University Press, 2015. Disponível em: https://doi.org/10.1017/S1743921314011600. Acesso em: 18 nov. 2024.
APA
Poidevin, F., Falceta-Gonçalves, D., Kowal, G., Dal Pino, E. M. de G., & Magalhães, A. M. (2015). Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog. In IAU Highlights of Astronomy, v. 16. Cambridge: Cambridge University Press. doi:10.1017/S1743921314011600
NLM
Poidevin F, Falceta-Gonçalves D, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog [Internet]. IAU Highlights of Astronomy, v. 16. 2015 ;[citado 2024 nov. 18 ] Available from: https://doi.org/10.1017/S1743921314011600
Vancouver
Poidevin F, Falceta-Gonçalves D, Kowal G, Dal Pino EM de G, Magalhães AM. Magnetic field components analysis of the SCUPOL 850 microns polarization data catalog [Internet]. IAU Highlights of Astronomy, v. 16. 2015 ;[citado 2024 nov. 18 ] Available from: https://doi.org/10.1017/S1743921314011600

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