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  • Fonte: 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: 14 out. 2025.
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/acd699
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: 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: 14 out. 2025.
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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 2025 out. 14 ] Available from: https://doi.org/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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/abefd7
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: 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: 14 out. 2025.
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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 2025 out. 14 ] Available from: https://doi.org/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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: 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: 14 out. 2025.
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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 2025 out. 14 ] Available from: https://doi.org/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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab63ca
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: 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: 14 out. 2025.
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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 2025 out. 14 ] Available from: https://doi.org/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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: 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: 14 out. 2025.
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab61fa
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: 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: 14 out. 2025.
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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
    • 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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab7a13
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: 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: 14 out. 2025.
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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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/abc331
  • Fonte: 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: 14 out. 2025.
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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
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: 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: 14 out. 2025.
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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
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf
  • Fonte: 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: 14 out. 2025.
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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
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://arxiv.org/pdf/1807.02604.pdf
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: 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: 14 out. 2025.
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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
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      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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aabba8
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      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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aabba8
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: 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: 14 out. 2025.
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      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
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6347
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: GALÁXIAS, EVOLUÇÃO ESTELAR, MAGNETOHIDRODINÂMICA

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      CAPRONI, Anderson et al. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, v. 838, n. 2, p. 1-9, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6002. Acesso em: 14 out. 2025.
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      Caproni, A., Lanfranchi, G. A., Baio, G. H. C., Kowal, G., & Falceta Gonçalves, D. A. (2017). Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, 838( 2), 1-9. doi:10.3847/1538-4357/aa6002
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      Caproni A, Lanfranchi GA, Baio GHC, Kowal G, Falceta Gonçalves DA. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.[citado 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
    • Vancouver

      Caproni A, Lanfranchi GA, Baio GHC, Kowal G, Falceta Gonçalves DA. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.[citado 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6002
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: CATÁLOGOS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS, CARBONO, ESPECTROSCOPIA

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      BEERS, Timothy C et al. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, v. 835, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 14 out. 2025.
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      Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, 835, 81. doi:10.3847/1538-4357/835/1/81
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      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
    • Vancouver

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: TURBULÊNCIA, MAGNETOHIDRODINÂMICA

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      KOWAL, Grzegorz et al. Statistics of reconnection-driven turbulence. The Astrophysical Journal, v. 838, n. 2, p. 1-13, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6001. Acesso em: 14 out. 2025.
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      Kowal, G., Falceta Gonçalves, D. A., Lazarian, A., & Vishniac, E. T. (2017). Statistics of reconnection-driven turbulence. The Astrophysical Journal, 838( 2), 1-13. doi:10.3847/1538-4357/aa6001
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      Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6001
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      Kowal G, Falceta Gonçalves DA, Lazarian A, Vishniac ET. Statistics of reconnection-driven turbulence [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-13.[citado 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/aa6001
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: JATOS (ASTRONOMIA), GALÁXIAS

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      SINGH, Chandra B e MIZUNO, Yosuke e DAL PINO, Elisabete Maria de Gouveia. Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection. The Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf. Acesso em: 14 out. 2025.
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      Singh, C. B., Mizuno, Y., & Dal Pino, E. M. de G. (2016). Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection. The Astrophysical Journal. doi:10.3847/0004-637X/824/1/48
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      Singh CB, Mizuno Y, Dal Pino EM de G. Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection [Internet]. The Astrophysical Journal. 2016 ;[citado 2025 out. 14 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf
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      Singh CB, Mizuno Y, Dal Pino EM de G. Spatial growth of current-driven instability in relativistic rotating jets and the search for magnetic reconnection [Internet]. The Astrophysical Journal. 2016 ;[citado 2025 out. 14 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: ASTROFÍSICA ESTELAR, INFRAVERMELHO

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      BARBOSA, C. L et al. A mid-infrared view of the high mass star formation region W51A. The Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf. Acesso em: 14 out. 2025.
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      Barbosa, C. L., Blum, R. D., Damineli Neto, A., Conti, P. S., & Gusmão, D. M. (2016). A mid-infrared view of the high mass star formation region W51A. The Astrophysical Journal. doi:10.3847/0004-637X/825/1/54
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      Barbosa CL, Blum RD, Damineli Neto A, Conti PS, Gusmão DM. A mid-infrared view of the high mass star formation region W51A [Internet]. The Astrophysical Journal. 2016 ;[citado 2025 out. 14 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf
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      Barbosa CL, Blum RD, Damineli Neto A, Conti PS, Gusmão DM. A mid-infrared view of the high mass star formation region W51A [Internet]. The Astrophysical Journal. 2016 ;[citado 2025 out. 14 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assuntos: ESTRELAS BINÁRIAS, ASTROFÍSICA ESTELAR

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      TEODORO, M et al. He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima. The Astrophysical Journal, v. 819, p. 131, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf. Acesso em: 14 out. 2025.
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      Teodoro, M., Damineli Neto, A., Hickel, G., Henrique, W., & Jablonski, F. (2016). He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima. The Astrophysical Journal, 819, 131. doi:10.3847/0004-637X/819/2/131
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      Teodoro M, Damineli Neto A, Hickel G, Henrique W, Jablonski F. He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima [Internet]. The Astrophysical Journal. 2016 ; 819 131.[citado 2025 out. 14 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf
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      Teodoro M, Damineli Neto A, Hickel G, Henrique W, Jablonski F. He II λ ‘lambda’ 4686 emission from the massive binary system in η ‘eta’car: constraints to the orbital elements and the nature of the periodic minima [Internet]. The Astrophysical Journal. 2016 ; 819 131.[citado 2025 out. 14 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf
  • Fonte: The Astrophysical Journal. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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      GAMA, Diana Renata Gonçalves et al. CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings. The Astrophysical Journal, v. 830, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf. Acesso em: 14 out. 2025.
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      Gama, D. R. G., Lépine, J. R. D., Mendoza, E., Wu, Y., & Yuan, J. (2016). CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings. The Astrophysical Journal, 830. doi:10.3847/0004-637X/830/2/57
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      Gama DRG, Lépine JRD, Mendoza E, Wu Y, Yuan J. CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings [Internet]. The Astrophysical Journal. 2016 ; 830[citado 2025 out. 14 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf
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      Gama DRG, Lépine JRD, Mendoza E, Wu Y, Yuan J. CO observations and investigation of triggered star formation toward the n10 infrared bubble and surroundings [Internet]. The Astrophysical Journal. 2016 ; 830[citado 2025 out. 14 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf

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