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Filtros : "The Astrophysical Journal: an international review of astronomy and astronomical physics" Removidos: "COSMOLOGIA" "Carciofi, Alex Cavaliéri" Limpar

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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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      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: 05 nov. 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

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      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 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/acd699

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      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 nov. 05 ] 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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/abefd7

  • 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: 05 nov. 2024.

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      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

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      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 2024 nov. 05 ] 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 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76

  • 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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] 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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] 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: 05 nov. 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

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      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 nov. 05 ] 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 nov. 05 ] 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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      KOWAL, Grzegorz et al. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?. The Astrophysical Journal, v. 892, n. 1, p. 01-15, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab7a13. Acesso em: 05 nov. 2024.

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      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

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      Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? [Internet]. The Astrophysical Journal. 2020 ; 892( 1): 01-15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13

    • Vancouver

      Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? [Internet]. The Astrophysical Journal. 2020 ; 892( 1): 01-15.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13

  • Artigo de periodico

    Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium (2020)

    Jesus, Lorena do Carmo ; González-Casanova, Diego F. ; Falceta Gonçalves, Diego Antonio ; Lazarian, Alex ; Jablonski, Francisco; Zhang, Jian-Fu; Ferreira, Ivan Soares ; Castro, Manuel L. Díaz; Yang, Bo

    Source: The Astrophysical Journal. Unidade: EACH

    Subjects: MAGNETOHIDRODINÂMICA, MEIO INTERESTELAR

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      JESUS, Lorena do Carmo et al. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, v. 905, n. 2, p. 01-12, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abc331. Acesso em: 05 nov. 2024.

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      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

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      Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/abc331

    • Vancouver

      Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/abc331

  • Artigo de periodico

    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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] 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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] 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, 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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      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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/ab5067

  • 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: 05 nov. 2024.

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      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

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      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. 05 ] 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. 05 ] 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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      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: 05 nov. 2024.

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      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

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      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. 05 ] 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. 05 ] 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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      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: 05 nov. 2024.

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      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

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      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 nov. 05 ] 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 nov. 05 ] 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

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      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: 05 nov. 2024.

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      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 nov. 05 ] 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 nov. 05 ] 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

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      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: 05 nov. 2024.

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      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 nov. 05 ] 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 nov. 05 ] 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

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      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: 05 nov. 2024.

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      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 nov. 05 ] 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 nov. 05 ] 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

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      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: 05 nov. 2024.

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      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 nov. 05 ] 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 nov. 05 ] 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

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      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: 05 nov. 2024.

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      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 nov. 05 ] 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 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aabba8

  • Artigo de periodico

    The 2014 X-Ray Minimum of η Carinae as Seen by Swift (2017)

    Corcoran, M F; Liburd, J.; Morris, D; Russell, C. M. P; Hamaguchi, K; Gull, T. R; Madura, Thomas I; Teodoro, M; Moffat, A F J; Richardson, N. D; Hillier, D.J; Damineli Neto, Augusto; Groh, J. H

    Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ESTRELAS, RAIOS X

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      CORCORAN, M F et al. The 2014 X-Ray Minimum of η Carinae as Seen by Swift. The Astrophysical Journal, v. 838, n. 1, p. 45, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6347. Acesso em: 05 nov. 2024.

    • APA

      Corcoran, M. F., Liburd, J., Morris, D., Russell, C. M. P., Hamaguchi, K., Gull, T. R., et al. (2017). The 2014 X-Ray Minimum of η Carinae as Seen by Swift. The Astrophysical Journal, 838( 1), 45. doi:10.3847/1538-4357/aa6347

    • NLM

      Corcoran MF, Liburd J, Morris D, Russell CMP, Hamaguchi K, Gull TR, Madura TI, Teodoro M, Moffat AFJ, Richardson ND, Hillier DJ, Damineli Neto A, Groh JH. The 2014 X-Ray Minimum of η Carinae as Seen by Swift [Internet]. The Astrophysical Journal. 2017 ;838( 1): 45.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aa6347

    • Vancouver

      Corcoran MF, Liburd J, Morris D, Russell CMP, Hamaguchi K, Gull TR, Madura TI, Teodoro M, Moffat AFJ, Richardson ND, Hillier DJ, Damineli Neto A, Groh JH. The 2014 X-Ray Minimum of η Carinae as Seen by Swift [Internet]. The Astrophysical Journal. 2017 ;838( 1): 45.[citado 2024 nov. 05 ] Available from: https://doi.org/10.3847/1538-4357/aa6347

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