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  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: ESTRELAS BINÁRIAS, RAIOS X, ASTROFÍSICA ESTELAR

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    • ABNT

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

    Assuntos: ASTROFÍSICA ESTELAR, NEBULOSAS, JATOS (ASTRONOMIA), EVOLUÇÃO ESTELAR

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    • ABNT

      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.
    • 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 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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    • 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: 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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    • ABNT

      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
    • NLM

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

    Assuntos: COSMOLOGIA, MATÉRIA ESCURA, SUPERNOVAS

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    • ABNT

      BROUT, D e LIMA, Marcos Vinicius Borges Teixeira. First Cosmology Results Using Type Ia Supernovae from the Dark Energy Survey: Photometric Pipeline and Light-curve Data Release. The Astrophysical Journal, v. 874, n. 1, p. 106/1-106/12, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab06c1. Acesso em: 14 out. 2025.
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      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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab06c1
  • Fonte: The Astrophysical Journal. Unidade: IF

    Assunto: NEUTRINOS

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    • 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: 14 out. 2025.
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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 2025 out. 14 ] 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 2025 out. 14 ] Available from: https://doi.org/10.3847/1538-4357/ab3a45
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: GALÁXIAS, EVOLUÇÃO ESTELAR, MAGNETOHIDRODINÂMICA

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    • ABNT

      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.
    • APA

      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
    • NLM

      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: EACH

    Assuntos: TURBULÊNCIA, MAGNETOHIDRODINÂMICA

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    • ABNT

      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
    • NLM

      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
    • Vancouver

      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: EACH

    Assuntos: MEIO INTERGALÁTICO, CAMPO MAGNÉTICO, TURBULÊNCIA, UNIVERSO PRIMORDIAL

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    • ABNT

      FALCETA GONÇALVES, Diego Antonio e KOWAL, Grzegorz. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media. The Astrophysical Journal, v. 808, n. 1, p. 1-15, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/65. Acesso em: 14 out. 2025.
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      Falceta Gonçalves, D. A., & Kowal, G. (2015). Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media. The Astrophysical Journal, 808( 1), 1-15. doi:10.1088/0004-637X/808/1/65
    • NLM

      Falceta Gonçalves DA, Kowal G. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media [Internet]. The Astrophysical Journal. 2015 ; 808( 1): 1-15.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/808/1/65
    • Vancouver

      Falceta Gonçalves DA, Kowal G. Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media [Internet]. The Astrophysical Journal. 2015 ; 808( 1): 1-15.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/808/1/65
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: GALÁXIAS, EVOLUÇÃO ESTELAR, HIDRODINÂMICA

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    • ABNT

      CAPRONI, Anderson et al. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, v. 805, n. ju 2015, p. 1-12, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/805/2/109. Acesso em: 14 out. 2025.
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      Caproni, A., Lanfranchi, G. A., Silva, A. L. da, & Falceta Gonçalves, D. A. (2015). Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor. The Astrophysical Journal, 805( ju 2015), 1-12. doi:10.1088/0004-637X/805/2/109
    • NLM

      Caproni A, Lanfranchi GA, Silva AL da, Falceta Gonçalves DA. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
    • Vancouver

      Caproni A, Lanfranchi GA, Silva AL da, Falceta Gonçalves DA. Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor [Internet]. The Astrophysical Journal. 2015 ; 805( ju 2015): 1-12.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/805/2/109
  • Fonte: The Astrophysical Journal. Unidade: IF

    Assunto: NÊUTRONS

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    • ABNT

      ABREU, P. et al. A source for point sources of EeV neutrons. The Astrophysical Journal, v. no2012, n. 2, p. 148-159, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/760/2/148. Acesso em: 14 out. 2025.
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      Abreu, P., Albuquerque, I. F. da M. e, Gouffon, P., & Tridapalli, D. B. (2012). A source for point sources of EeV neutrons. The Astrophysical Journal, no2012( 2), 148-159. doi:10.1088/0004-637X/760/2/148
    • NLM

      Abreu P, Albuquerque IF da M e, Gouffon P, Tridapalli DB. A source for point sources of EeV neutrons [Internet]. The Astrophysical Journal. 2012 ; no2012( 2): 148-159.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/760/2/148
    • Vancouver

      Abreu P, Albuquerque IF da M e, Gouffon P, Tridapalli DB. A source for point sources of EeV neutrons [Internet]. The Astrophysical Journal. 2012 ; no2012( 2): 148-159.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/760/2/148
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assunto: ASTROFÍSICA ESTELAR

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      FALCETA GONÇALVES, Diego Antonio e LAZARIAN, A. Evolution and lifetime of transient clumps in the turbulent interstellar medium. The Astrophysical Journal, v. 735, n. 2, p. 1-7, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/735/2/99. Acesso em: 14 out. 2025.
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      Falceta Gonçalves, D. A., & Lazarian, A. (2011). Evolution and lifetime of transient clumps in the turbulent interstellar medium. The Astrophysical Journal, 735( 2), 1-7. doi:10.1088/0004-637X/735/2/99
    • NLM

      Falceta Gonçalves DA, Lazarian A. Evolution and lifetime of transient clumps in the turbulent interstellar medium [Internet]. The Astrophysical Journal. 2011 ; 735( 2): 1-7.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99
    • Vancouver

      Falceta Gonçalves DA, Lazarian A. Evolution and lifetime of transient clumps in the turbulent interstellar medium [Internet]. The Astrophysical Journal. 2011 ; 735( 2): 1-7.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99
  • Fonte: The Astrophysical Journal. Unidade: EACH

    Assuntos: ASTROFÍSICA ESTELAR, NEBULOSAS, MEIO INTERGALÁTICO

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      MONTEIRO, Hektor e FALCETA GONÇALVES, Diego Antonio. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40. The Astrophysical Journal, v. 738, n. 2, p. 1-10, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/738/2/174. Acesso em: 14 out. 2025.
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      Monteiro, H., & Falceta Gonçalves, D. A. (2011). Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40. The Astrophysical Journal, 738( 2), 1-10. doi:10.1088/0004-637X/738/2/174
    • NLM

      Monteiro H, Falceta Gonçalves DA. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 [Internet]. The Astrophysical Journal. 2011 ; 738( 2): 1-10.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/738/2/174
    • Vancouver

      Monteiro H, Falceta Gonçalves DA. Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40 [Internet]. The Astrophysical Journal. 2011 ; 738( 2): 1-10.[citado 2025 out. 14 ] Available from: https://doi.org/10.1088/0004-637X/738/2/174

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