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Artigo de periodico
Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales (2023)
Torrejón, Tania Elizabeth Medina ; Pino, Elisabete Maria de Gouveia Dal ; Kowal, Grzegorz
Source: The Astrophysical Journal. Unidades: IAG, EACH
Assunto: ASTROFÍSICA
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ABNT
TORREJÓN, Tania Elizabeth Medina e PINO, Elisabete Maria de Gouveia Dal e KOWAL, Grzegorz. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales. The Astrophysical Journal, v. 952, n. 2, p. 01-11, 2023Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/acd699. Acesso em: 03 out. 2024.
APA
Torrejón, T. E. M., Pino, E. M. de G. D., & Kowal, G. (2023). Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales. The Astrophysical Journal, 952( 2), 01-11. doi:10.3847/1538-4357/acd699
NLM
Torrejón TEM, Pino EM de GD, Kowal G. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales [Internet]. The Astrophysical Journal. 2023 ; 952( 2): 01-11.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/acd699
Vancouver
Torrejón TEM, Pino EM de GD, Kowal G. Particle acceleration by magnetic reconnection in relativistic jets: the transition from small to large scales [Internet]. The Astrophysical Journal. 2023 ; 952( 2): 01-11.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/acd699
Artigo de periodico
X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions (2021)
Ortiz, Roberto Pereira ; Guerrero, Martín A
Source: The Astrophysical Journal. Unidade: EACH
Subjects: ESTRELAS BINÁRIAS, RAIOS X, ASTROFÍSICA ESTELAR
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ORTIZ, Roberto Pereira e GUERRERO, Martín A. X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions. The Astrophysical Journal, v. 912, n. 2, p. 01-14, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abefd7. Acesso em: 03 out. 2024.
APA
Ortiz, R. P., & Guerrero, M. A. (2021). X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions. The Astrophysical Journal, 912( 2), 01-14. doi:10.3847/1538-4357/abefd7
NLM
Ortiz RP, Guerrero MA. X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions [Internet]. The Astrophysical Journal. 2021 ; 912( 2): 01-14.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/abefd7
Vancouver
Ortiz RP, Guerrero MA. X-Ray AGB Stars in the 4XMM-DR9 Catalog: Further Evidence for Companions [Internet]. The Astrophysical Journal. 2021 ; 912( 2): 01-14.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/abefd7
Artigo de periodico
Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205 (2020)
Catalán-Torrecill, C ; Castilho-Morales, Á ; Coelho, Paula Rodrigues Teixeira
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MEIO INTERESTELAR, ESPECTROSCOPIA
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CATALÁN-TORRECILL, C e CASTILHO-MORALES, Á e COELHO, Paula Rodrigues Teixeira. Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205. The Astrophysical Journal, v. 890, p. 5, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab63ca. Acesso em: 03 out. 2024.
APA
Catalán-Torrecill, C., Castilho-Morales, Á., & Coelho, P. R. T. (2020). Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205. The Astrophysical Journal, 890, 5. doi:10.3847/1538-4357/ab63ca
NLM
Catalán-Torrecill C, Castilho-Morales Á, Coelho PRT. Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205 [Internet]. The Astrophysical Journal. 2020 ; 890 5.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
Vancouver
Catalán-Torrecill C, Castilho-Morales Á, Coelho PRT. Spatially resolved analysis of neutral winds, stars, and ionized gas kinematics with megara/gtc: new insights on the nearby galaxy ugc 10205 [Internet]. The Astrophysical Journal. 2020 ; 890 5.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
Artigo de periodico
Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster (2020)
Souza, S. O ; Kerber, Leandro de Oliveira ; Barbuy, Beatriz Leonor Silveira ; Pérez-Villegas, A ; Oliveira, R. A. P. ; Nardiello, D
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES
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SOUZA, S. O et al. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster. The Astrophysical Journal, v. 890, p. 13 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6a0f. Acesso em: 03 out. 2024.
APA
Souza, S. O., Kerber, L. de O., Barbuy, B. L. S., Pérez-Villegas, A., Oliveira, R. A. P., & Nardiello, D. (2020). Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster. The Astrophysical Journal, 890, 13 2020. doi:10.3847/1538-4357/ab6a0f
NLM
Souza SO, Kerber L de O, Barbuy BLS, Pérez-Villegas A, Oliveira RAP, Nardiello D. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster [Internet]. The Astrophysical Journal. 2020 ; 890 13 2020.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
Vancouver
Souza SO, Kerber L de O, Barbuy BLS, Pérez-Villegas A, Oliveira RAP, Nardiello D. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster [Internet]. The Astrophysical Journal. 2020 ; 890 13 2020.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
Artigo de periodico
Space Velocity and Time Span of Jets in Planetary Nebulae (2020)
Guerrero, Martín A ; Rechy-García, Jackeline Suzett ; Ortiz, Roberto Pereira
Source: The Astrophysical Journal. Unidade: EACH
Subjects: ASTROFÍSICA ESTELAR, NEBULOSAS, JATOS (ASTRONOMIA), EVOLUÇÃO ESTELAR
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GUERRERO, Martín A e RECHY-GARCÍA, Jackeline Suzett e ORTIZ, Roberto Pereira. Space Velocity and Time Span of Jets in Planetary Nebulae. The Astrophysical Journal, v. 890, n. 1, p. 01-14, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab61fa. Acesso em: 03 out. 2024.
APA
Guerrero, M. A., Rechy-García, J. S., & Ortiz, R. P. (2020). Space Velocity and Time Span of Jets in Planetary Nebulae. The Astrophysical Journal, 890( 1), 01-14. doi:10.3847/1538-4357/ab61fa
NLM
Guerrero MA, Rechy-García JS, Ortiz RP. Space Velocity and Time Span of Jets in Planetary Nebulae [Internet]. The Astrophysical Journal. 2020 ; 890( 1): 01-14.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab61fa
Vancouver
Guerrero MA, Rechy-García JS, Ortiz RP. Space Velocity and Time Span of Jets in Planetary Nebulae [Internet]. The Astrophysical Journal. 2020 ; 890( 1): 01-14.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab61fa
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: 03 out. 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 out. 03 ] 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 out. 03 ] 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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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: 03 out. 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 out. 03 ] 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 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/abc331
Artigo de periodico
Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood (2019)
Michtchenko, Tatiana Alexandrovna; Barros, Douglas A; Perez-Villegas, Angeles; Lépine, Jacques Raymond Daniel
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS ESPIRAIS, ESTRUTURA DA GALÁXIA
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MICHTCHENKO, Tatiana Alexandrovna et al. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood. The Astrophysical Journal, v. 876, n. 1, p. 36/1-36/7, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab11cd. Acesso em: 03 out. 2024.
APA
Michtchenko, T. A., Barros, D. A., Perez-Villegas, A., & Lépine, J. R. D. (2019). Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood. The Astrophysical Journal, 876( 1), 36/1-36/7. doi:10.3847/1538-4357/ab11cd
NLM
Michtchenko TA, Barros DA, Perez-Villegas A, Lépine JRD. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood [Internet]. The Astrophysical Journal. 2019 ; 876( 1): 36/1-36/7.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
Vancouver
Michtchenko TA, Barros DA, Perez-Villegas A, Lépine JRD. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood [Internet]. The Astrophysical Journal. 2019 ; 876( 1): 36/1-36/7.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
Artigo de periodico
Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} (2019)
Rodríguez-Ramírez, Juan Carlos ; Dal Pino, Elisabete Maria de Gouveia ; Batista, Rafael Alves
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, MAGNETOHIDRODINÂMICA, CENTRO GALÁCTICO
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RODRÍGUEZ-RAMÍREZ, Juan Carlos e DAL PINO, Elisabete Maria de Gouveia e BATISTA, Rafael Alves. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, v. 879, n. 1, p. 6/1-6/10, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab212e. Acesso em: 03 out. 2024.
APA
Rodríguez-Ramírez, J. C., Dal Pino, E. M. de G., & Batista, R. A. (2019). Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, 879( 1), 6/1-6/10. doi:10.3847/1538-4357/ab212e
NLM
Rodríguez-Ramírez JC, Dal Pino EM de G, Batista RA. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} [Internet]. The Astrophysical Journal. 2019 ; 879( 1): 6/1-6/10.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
Vancouver
Rodríguez-Ramírez JC, Dal Pino EM de G, Batista RA. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*} [Internet]. The Astrophysical Journal. 2019 ; 879( 1): 6/1-6/10.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
Artigo de periodico
First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release (2019)
Brout, D ; Lima, Marcos Vinicius Borges Teixeira
Source: The Astrophysical Journal. Unidade: IF
Subjects: COSMOLOGIA, MATÉRIA ESCURA, SUPERNOVAS
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ABNT
BROUT, D e LIMA, Marcos Vinicius Borges Teixeira. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, v. 874, n. 1, p. 106/1-106/12, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab06c1. Acesso em: 03 out. 2024.
APA
Brout, D., & Lima, M. V. B. T. (2019). First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, 874( 1), 106/1-106/12. doi:10.3847/1538-4357/ab06c1
NLM
Brout D, Lima MVBT. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release [Internet]. The Astrophysical Journal. 2019 ; 874( 1): 106/1-106/12.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1
Vancouver
Brout D, Lima MVBT. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release [Internet]. The Astrophysical Journal. 2019 ; 874( 1): 106/1-106/12.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1
Artigo de periodico
Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations (2019)
Raphaldini, Breno; Teruya, Andre Seiji; Raupp, Carlos Frederico Mendonça ; Bustamante, Miguel D
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MAGNETOHIDRODINÂMICA, ONDAS DE ROSSBY, ATIVIDADE SOLAR
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ABNT
RAPHALDINI, Breno et al. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations. The Astrophysical Journal, v. 887, n. 1, p. 17, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab5067. Acesso em: 03 out. 2024.
APA
Raphaldini, B., Teruya, A. S., Raupp, C. F. M., & Bustamante, M. D. (2019). Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations. The Astrophysical Journal, 887( 1), 17. doi:10.3847/1538-4357/ab5067
NLM
Raphaldini B, Teruya AS, Raupp CFM, Bustamante MD. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations [Internet]. The Astrophysical Journal. 2019 ; 887( 1): 17.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab5067
Vancouver
Raphaldini B, Teruya AS, Raupp CFM, Bustamante MD. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations [Internet]. The Astrophysical Journal. 2019 ; 887( 1): 17.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab5067
Artigo de periodico
The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos (2019)
Silva, Leandro Beraldo e; De Siqueira Pedra, Walter ; Valluri, Monica; Sodré Júnior, Laerte; Bru, Jean-Bernard
Source: The Astrophysical Journal. Unidades: IAG, IF
Subjects: GALÁXIAS, MECÂNICA QUÂNTICA, MATEMÁTICA APLICADA, COSMOLOGIA
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ABNT
SILVA, Leandro Beraldo e et al. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos. The Astrophysical Journal, v. 870, n. 2, p. 128, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf397. Acesso em: 03 out. 2024.
APA
Silva, L. B. e, De Siqueira Pedra, W., Valluri, M., Sodré Júnior, L., & Bru, J. -B. (2019). The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos. The Astrophysical Journal, 870( 2), 128. doi:10.3847/1538-4357/aaf397
NLM
Silva LB e, De Siqueira Pedra W, Valluri M, Sodré Júnior L, Bru J-B. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos [Internet]. The Astrophysical Journal. 2019 ;870( 2): 128.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/aaf397
Vancouver
Silva LB e, De Siqueira Pedra W, Valluri M, Sodré Júnior L, Bru J-B. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos [Internet]. The Astrophysical Journal. 2019 ;870( 2): 128.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/aaf397
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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ABNT
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: 03 out. 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 out. 03 ] 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 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
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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ABNT
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: 03 out. 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 out. 03 ] 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 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
Artigo de periodico
Integrated Spectra of Milky Way Globular Clusters (2019)
Moura, T. C; Trevisan, M; Barbuy, Beatriz Leonor Silveira; Rossi, Silvia Cristina Fernandes
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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ABNT
MOURA, T. C et al. Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab3eb6. Acesso em: 03 out. 2024.
APA
Moura, T. C., Trevisan, M., Barbuy, B. L. S., & Rossi, S. C. F. (2019). Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab3eb6
NLM
Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
Vancouver
Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
Artigo de periodico
A DECam search for explosive optical transients associated with IceCube neutrino alerts (2019)
Morgan, R; Lima, Marcos Vinicius Borges Teixeira
Source: The Astrophysical Journal. Unidade: IF
Assunto: NEUTRINOS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MORGAN, R e LIMA, Marcos Vinicius Borges Teixeira. A DECam search for explosive optical transients associated with IceCube neutrino alerts. The Astrophysical Journal, v. 883, n. 2, p. 1-18, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab3a45. Acesso em: 03 out. 2024.
APA
Morgan, R., & Lima, M. V. B. T. (2019). A DECam search for explosive optical transients associated with IceCube neutrino alerts. The Astrophysical Journal, 883( 2), 1-18. doi:10.3847/1538-4357/ab3a45
NLM
Morgan R, Lima MVBT. A DECam search for explosive optical transients associated with IceCube neutrino alerts [Internet]. The Astrophysical Journal. 2019 ; 883( 2): 1-18.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab3a45
Vancouver
Morgan R, Lima MVBT. A DECam search for explosive optical transients associated with IceCube neutrino alerts [Internet]. The Astrophysical Journal. 2019 ; 883( 2): 1-18.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/ab3a45
Artigo de periodico
G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN (2018)
Mendoza, Edgar; Bronfman, Leonardo; Duronea, Nicolas U; Lépine, Jacques Raymond Daniel; Finger, Ricardo; Merello, Manuel; Caimapo, Carlos Hervías; Gama, Diana Renata Gonçalves; Ake-Nyman, Lars
Source: The Astrophysical Journal. Unidade: IAG
Assunto: MEIO INTERESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MENDOZA, Edgar et al. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN. The Astrophysical Journal, v. 853, p. 152, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaa1ec. Acesso em: 03 out. 2024.
APA
Mendoza, E., Bronfman, L., Duronea, N. U., Lépine, J. R. D., Finger, R., Merello, M., et al. (2018). G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN. The Astrophysical Journal, 853, 152. doi:10.3847/1538-4357/aaa1ec
NLM
Mendoza E, Bronfman L, Duronea NU, Lépine JRD, Finger R, Merello M, Caimapo CH, Gama DRG, Ake-Nyman L. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN [Internet]. The Astrophysical Journal. 2018 ; 853 152.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
Vancouver
Mendoza E, Bronfman L, Duronea NU, Lépine JRD, Finger R, Merello M, Caimapo CH, Gama DRG, Ake-Nyman L. G331.512-0.103: An Interstellar Laboratory for Molecular Synthesis I. The Ortho-to-para Ratios for CH3OH and CH3CN [Internet]. The Astrophysical Journal. 2018 ; 853 152.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
Artigo de periodico
Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams* (2018)
Kerber, L. O; Nardiello, D; Barbuy, Beatriz Leonor Silveira; Bica, E
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, POPULAÇÕES ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
KERBER, L. O et al. Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams*. The Astrophysical Journal, v. 853, p. 15, 2018Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf. Acesso em: 03 out. 2024.
APA
Kerber, L. O., Nardiello, D., Barbuy, B. L. S., & Bica, E. (2018). Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams*. The Astrophysical Journal, 853, 15. doi:10.3847/1538-4357/aaa3fc
NLM
Kerber LO, Nardiello D, Barbuy BLS, Bica E. Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams* [Internet]. The Astrophysical Journal. 2018 ; 853 15.[citado 2024 out. 03 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf
Vancouver
Kerber LO, Nardiello D, Barbuy BLS, Bica E. Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams* [Internet]. The Astrophysical Journal. 2018 ; 853 15.[citado 2024 out. 03 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf
Artigo de periodico
NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN (2018)
SILVA, Patricia da; Steiner, João Evangelista; Menezes, R.B
Source: The Astrophysical Journal. Unidade: IAG
Assunto: GALÁXIAS ATIVAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SILVA, Patricia da e STEINER, João Evangelista e MENEZES, R.B. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN. The Astrophysical Journal, v. 861, p. 83, 2018Tradução . . Disponível em: https://arxiv.org/pdf/1807.02604.pdf. Acesso em: 03 out. 2024.
APA
SILVA, P. da, Steiner, J. E., & Menezes, R. B. (2018). NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN. The Astrophysical Journal, 861, 83. doi:10.3847/1538-4357/aac6e3
NLM
SILVA P da, Steiner JE, Menezes RB. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN [Internet]. The Astrophysical Journal. 2018 ; 861 83.[citado 2024 out. 03 ] Available from: https://arxiv.org/pdf/1807.02604.pdf
Vancouver
SILVA P da, Steiner JE, Menezes RB. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN [Internet]. The Astrophysical Journal. 2018 ; 861 83.[citado 2024 out. 03 ] Available from: https://arxiv.org/pdf/1807.02604.pdf
Artigo de periodico
Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs (2018)
Kadowaki, L. H. S; Dal Pino, Elisabete Maria de Gouveia; Singh, Chandra B
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, GALÁXIAS ATIVAS, RAIOS GAMA, MAGNETISMO, ESTRELAS BINÁRIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
KADOWAKI, L. H. S e DAL PINO, Elisabete Maria de Gouveia e SINGH, Chandra B. Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs. The Astrophysical Journal, v. 857, p. 146, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aabba8. Acesso em: 03 out. 2024.
APA
Kadowaki, L. H. S., Dal Pino, E. M. de G., & Singh, C. B. (2018). Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs. The Astrophysical Journal, 857, 146. doi:10.3847/1538-4357/aabba8
NLM
Kadowaki LHS, Dal Pino EM de G, Singh CB. Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs [Internet]. The Astrophysical Journal. 2018 ; 857 146.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/aabba8
Vancouver
Kadowaki LHS, Dal Pino EM de G, Singh CB. Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs [Internet]. The Astrophysical Journal. 2018 ; 857 146.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/1538-4357/aabba8

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