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Artigo de periodico
The BINGO/ABDUS Project: Forecast for Cosmological Parameters from a Mock Fast Radio Burst Survey (2025)
Zhang, Xue ; Hoerning, Gabriel A ; Abdalla, Filipe B ; Abdalla, Elcio
Source: The Astrophysical Journal. Unidade: IF
Assunto: COSMOLOGIA
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ABNT
ZHANG, Xue et al. The BINGO/ABDUS Project: Forecast for Cosmological Parameters from a Mock Fast Radio Burst Survey. The Astrophysical Journal, 2025Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/adfa11. Acesso em: 25 abr. 2026.
APA
Zhang, X., Hoerning, G. A., Abdalla, F. B., & Abdalla, E. (2025). The BINGO/ABDUS Project: Forecast for Cosmological Parameters from a Mock Fast Radio Burst Survey. The Astrophysical Journal. doi:https://doi.org/10.3847/1538-4357/adfa11
NLM
Zhang X, Hoerning GA, Abdalla FB, Abdalla E. The BINGO/ABDUS Project: Forecast for Cosmological Parameters from a Mock Fast Radio Burst Survey [Internet]. The Astrophysical Journal. 2025 ;[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/adfa11
Vancouver
Zhang X, Hoerning GA, Abdalla FB, Abdalla E. The BINGO/ABDUS Project: Forecast for Cosmological Parameters from a Mock Fast Radio Burst Survey [Internet]. The Astrophysical Journal. 2025 ;[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/adfa11
Artigo de periodico
Constraints on interacting dark energy revisited:: Implications for the Hubble tension (2025)
Hoerning, Gabriel A ; Landim, Ricardo G ; Ponte, Luiza O. ; Rolim, Raphael P. ; Abdalla, Filipe B ; Abdalla, Elcio
Source: The Astrophysical Journal. Unidades: IF, IAG
Assunto: COSMOLOGIA
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HOERNING, Gabriel A et al. Constraints on interacting dark energy revisited:: Implications for the Hubble tension. The Astrophysical Journal, 2025Tradução . . Disponível em: https://doi.org/10.1103/6zrh-8fmv. Acesso em: 25 abr. 2026.
APA
Hoerning, G. A., Landim, R. G., Ponte, L. O., Rolim, R. P., Abdalla, F. B., & Abdalla, E. (2025). Constraints on interacting dark energy revisited:: Implications for the Hubble tension. The Astrophysical Journal. doi:https://doi.org/10.1103/6zrh-8fmv
NLM
Hoerning GA, Landim RG, Ponte LO, Rolim RP, Abdalla FB, Abdalla E. Constraints on interacting dark energy revisited:: Implications for the Hubble tension [Internet]. The Astrophysical Journal. 2025 ;[citado 2026 abr. 25 ] Available from: https://doi.org/10.1103/6zrh-8fmv
Vancouver
Hoerning GA, Landim RG, Ponte LO, Rolim RP, Abdalla FB, Abdalla E. Constraints on interacting dark energy revisited:: Implications for the Hubble tension [Internet]. The Astrophysical Journal. 2025 ;[citado 2026 abr. 25 ] Available from: https://doi.org/10.1103/6zrh-8fmv
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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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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] 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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/abefd7
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
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. ; Gonçalves, Diego Antonio Falceta ; 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: 25 abr. 2026.
APA
Jesus, L. do C., González-Casanova, D. F., Gonçalves, D. A. F., 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, Gonçalves DAF, 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/abc331
Vancouver
Jesus L do C, González-Casanova DF, Gonçalves DAF, 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/abc331
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab61fa
Artigo de periodico
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters (2020)
Oliveira, R. A. P. ; Souza, S. O ; keber, L. O ; Barbuy, Beatriz Leonor Silveira
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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OLIVEIRA, R. A. P. et al. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6f76. Acesso em: 25 abr. 2026.
APA
Oliveira, R. A. P., Souza, S. O., keber, L. O., & Barbuy, B. L. S. (2020). The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab6f76
NLM
Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
Vancouver
Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
Artigo de periodico
Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? (2020)
Kowal, Grzegorz ; Gonçalves, Diego Antonio Falceta ; 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: 25 abr. 2026.
APA
Kowal, G., Gonçalves, D. A. F., 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, Gonçalves DAF, 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
Vancouver
Kowal G, Gonçalves DAF, 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab224a
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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ABNT
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab2460
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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ABNT
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab212e
Artigo de periodico
Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations (2019)
Raphaldini, Breno; Teruya, André Seiji Watake ; Raupp, Carlos Frederico Mendonça ; Bustamante, Miguel D
Source: The Astrophysical Journal. Unidade: IAG
Subjects: MAGNETOHIDRODINÂMICA, ONDAS DE ROSSBY, ATIVIDADE SOLAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 25 abr. 2026.
APA
Raphaldini, B., Teruya, A. S. W., 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 ASW, 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab5067
Vancouver
Raphaldini B, Teruya ASW, 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab5067
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/aaf397
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab3a45
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: 25 abr. 2026.
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 2026 abr. 25 ] 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 2026 abr. 25 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf

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