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  • Source: The Astrophysical Journal. Unidade: EACH

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

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      GUERRERO, Martín A; RECHY-GARCÍA, Jackeline Suzett; ORTIZ, Roberto Pereira. Space Velocity and Time Span of Jets in Planetary Nebulae. The Astrophysical Journal, Philadelphia, v. 890, n. 1, p. 01-14, 2020. Disponível em: < http://doi.org/10.3847/1538-4357/ab61fa > DOI: 10.3847/1538-4357/ab61fa.
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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
    • 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.Available from: http://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.Available from: http://doi.org/10.3847/1538-4357/ab61fa
  • Source: The Astrophysical Journal. Unidade: EACH

    Subjects: TURBULÊNCIA, ASTROFÍSICA

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      KOWAL, Grzegorz; FALCETA GONÇALVES, Diego Antonio; LAZARIAN, Alex; VISHNIAC, Ethan T. Kelvin–Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection? The Astrophysical Journal, Philadelphia, v. 892, n. 1, p. 01-15, 2020. Disponível em: < https://doi.org/10.3847/1538-4357/ab7a13 > DOI: 10.3847/1538-4357/ab7a13.
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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.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.Available from: https://doi.org/10.3847/1538-4357/ab7a13
  • Source: The Astrophysical Journal. Unidade: EACH

    Subjects: MAGNETOHIDRODINÂMICA, MEIO INTERESTELAR

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      JESUS, Lorena do Carmo; GONZÁLEZ-CASANOVA, Diego F.; FALCETA GONÇALVES, Diego Antonio; et al. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, Philadelphia, v. 905, n. 2, p. 01-12, 2020. Disponível em: < https://doi.org/10.3847/1538-4357/abc331 > DOI: 10.3847/1538-4357/abc331.
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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.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.Available from: https://doi.org/10.3847/1538-4357/abc331
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: DISCOS DE ACRESÇÃO, MAGNETOHIDRODINÂMICA, CENTRO GALÁCTICO

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      RODRÍGUEZ-RAMÍREZ, Juan Carlos; DAL PINO, Elisabete Maria de Gouveia; BATISTA, Rafael Alves. Very-high-energy Emission from Magnetic Reconnection in the Radiative-inefficient Accretion Flow of SgrA{*}. The Astrophysical Journal, Oxford, v. 879, n. 1, p. 6/1-6/10, 2019. Disponível em: < https://doi.org/10.3847/1538-4357/ab212e > DOI: 10.3847/1538-4357/ab212e.
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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
    • 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.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.Available from: https://doi.org/10.3847/1538-4357/ab212e
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS ESPIRAIS, ESTRUTURA DA GALÁXIA

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      MICHTCHENKO, Tatiana Alexandrovna; BARROS, Douglas A; PEREZ-VILLEGAS, Angeles; LÉPINE, Jacques Raymond Daniel. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood. The Astrophysical Journal, Oxford, v. 876, n. 1, p. 36/1-36/7, 2019. Disponível em: < https://doi.org/10.3847/1538-4357/ab11cd > DOI: 10.3847/1538-4357/ab11cd.
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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.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.Available from: https://doi.org/10.3847/1538-4357/ab11cd
  • Source: The Astrophysical Journal. Unidade: IF

    Subjects: MATÉRIA ESCURA, SUPERNOVAS, COSMOLOGIA

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      BROUT, D; 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, Oxford, v. 874, n. 1, p. 106/1-106/12, 2019. Disponível em: < https://doi.org/10.3847/1538-4357/ab06c1 > DOI: 10.3847/1538-4357/ab06c1.
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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
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      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.Available from: https://doi.org/10.3847/1538-4357/ab06c1
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      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.Available from: https://doi.org/10.3847/1538-4357/ab06c1
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: MAGNETOHIDRODINÂMICA, ONDAS DE ROSSBY, ATIVIDADE SOLAR

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      RAPHALDINI, Breno; TERUYA, Andre Seiji; RAUPP, Carlos Frederico Mendonça; BUSTAMANTE, Miguel D. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations. The Astrophysical Journal, Oxford, v. 887, n. 1, p. 17, 2019. Disponível em: < https://doi.org/10.3847/1538-4357/ab5067 > DOI: 10.3847/1538-4357/ab5067.
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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
    • NLM

      Raphaldini B, Teruya AS, Raupp CFM, Bustamante MD. Nonlinear Rossby Wave-Wave and Wave-Mean Flow Theory for Long-term Solar Cycle Modulations [Internet]. The Astrophysical Journal. 2019 ; 887( 1): 17.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.Available from: https://doi.org/10.3847/1538-4357/ab5067
  • Source: The Astrophysical Journal. Unidades: IAG, IF

    Subjects: GALÁXIAS, MECÂNICA QUÂNTICA, MATEMÁTICA APLICADA, COSMOLOGIA

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      SILVA, Leandro Beraldo e; PEDRA, Walter Alberto de Siqueira; VALLURI, Monica; SODRÉ JÚNIOR, Laerte; BRU, Jean-Bernard. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos. The Astrophysical Journal, Bristol, v. 870, n. 2, p. 128, 2019. Disponível em: < https://iopscience.iop.org/article/10.3847/1538-4357/aaf397/pdf > DOI: 10.3847/1538-4357/aaf397.
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      Silva, L. B. e, Pedra, W. A. de S., 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, Pedra WA de S, 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.Available from: https://iopscience.iop.org/article/10.3847/1538-4357/aaf397/pdf
    • Vancouver

      Silva LB e, Pedra WA de S, 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.Available from: https://iopscience.iop.org/article/10.3847/1538-4357/aaf397/pdf
  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Subjects: PLASMA, ONDAS DE CHOQUE, CAMPO MAGNÉTICO, SOL

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      PÁEZ, A.; JATENCO-PEREIRA, Vera; GONÇALVES, Diego Antonio Falceta; OPHER, M. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration. The Astrophysical Journal, Philadelphia, v. 879, n. 2, p. 01-09, 2019. Disponível em: < http://dx.doi.org/10.3847/1538-4357/ab2460 > DOI: 10.3847/1538-4357/ab2460.
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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.Available from: http://dx.doi.org/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.Available from: http://dx.doi.org/10.3847/1538-4357/ab2460
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: CAMPO MAGNÉTICO, ASTROFÍSICA SOLAR

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      GUERRERO, G; ZAIRE, B; SMOLARKIEWICZ, P. K; et al. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? The Astrophysical Journal, Oxford, v. 880, n. 1, p. 6/1-6/20, 2019. Disponível em: < https://doi.org/10.3847/1538-4357/ab224a > DOI: 10.3847/1538-4357/ab224a.
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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.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.Available from: https://doi.org/10.3847/1538-4357/ab224a
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES

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      MOURA, T. C; TREVISAN, M; BARBUY, Beatriz Leonor Silveira; ROSSI, Silvia Cristina Fernandes. Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, Oxford, v. No, n. 1, p. 28/1-28/23, 2019. Disponível em: < https://doi.org/10.3847/1538-4357/ab3eb6 > DOI: 10.3847/1538-4357/ab3eb6.
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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.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.Available from: https://doi.org/10.3847/1538-4357/ab3eb6
  • Source: The Astrophysical Journal. Unidade: IF

    Assunto: NEUTRINOS

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      MORGAN, R; LIMA, Marcos Vinicius Borges Teixeira. A DECam search for explosive optical transients associated with IceCube neutrino alerts. The Astrophysical Journal, Washington, v. 883, n. 2, p. 1-18, 2019. DOI: 10.3847/1538-4357/ab3a45.
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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
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      Morgan R, Lima MVBT. A DECam search for explosive optical transients associated with IceCube neutrino alerts. The Astrophysical Journal. 2019 ; 883( 2): 1-18.
    • Vancouver

      Morgan R, Lima MVBT. A DECam search for explosive optical transients associated with IceCube neutrino alerts. The Astrophysical Journal. 2019 ; 883( 2): 1-18.
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, POPULAÇÕES ESTELARES

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      KERBER, L. O; NARDIELLO, D; BARBUY, Beatriz Leonor Silveira; BICA, E. Ages of the bulge globular clusters NGC 6522 and NGC 6626 (M28) from HST proper-motion-cleaned color–magnitude diagrams*. The Astrophysical Journal, Washington, v. 853, p. 15, 2018. Disponível em: < http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf > DOI: 10.3847/1538-4357/aaa3fc.
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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.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.Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Assunto: MEIO INTERESTELAR

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      MENDOZA, Edgar; BRONFMAN, Leonardo; DURONEA, Nicolas U; 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, Bristol, v. 853, p. 152, 2018. Disponível em: < https://doi.org/10.3847/1538-4357/aaa1ec > DOI: 10.3847/1538-4357/aaa1ec.
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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, Ake-Nyman L, Gama DRG. 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.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, Ake-Nyman L, Gama DRG. 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.Available from: https://doi.org/10.3847/1538-4357/aaa1ec
  • Source: The Astrophysical Journal. Unidade: IAG

    Assunto: GALÁXIAS ATIVAS

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      SILVA, Patricia da; STEINER, João Evangelista; MENEZES, R.B. NGC 6744: a nearby Milky Way twin with a very low-luminosity AGN. The Astrophysical Journal, Bristol, v. 861, p. 83, 2018. Disponível em: < https://arxiv.org/pdf/1807.02604.pdf > DOI: 10.3847/1538-4357/aac6e3.
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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.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.Available from: https://arxiv.org/pdf/1807.02604.pdf
  • 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; DAL PINO, Elisabete Maria de Gouveia; 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, Bristol, v. 857, p. 146, 2018. Disponível em: < https://doi.org/10.3847/1538-4357/aabba8 > DOI: https://doi.org/10.3847/1538-4357/aabba8.
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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:https://doi.org/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.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.Available from: https://doi.org/10.3847/1538-4357/aabba8
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ESTRELAS, RAIOS X

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    • ABNT

      CORCORAN, M F; LIBURD, J.; MORRIS, D; et al. The 2014 X-Ray Minimum of η Carinae as Seen by Swift. The Astrophysical Journal, Bristol, v. 838, n. 1, p. 45, 2017. Disponível em: < https://doi.org/10.3847/1538-4357/aa6347 > DOI: 10.3847/1538-4357/aa6347.
    • 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.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.Available from: https://doi.org/10.3847/1538-4357/aa6347
  • Source: The Astrophysical Journal. Unidade: EACH

    Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR, MAGNETOHIDRODINÂMICA

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    • ABNT

      CAPRONI, Anderson; KOWAL, Grzegorz; FALCETA GONÇALVES, Diego Antonio; LANFRANCHI, Gustavo Amaral; BAIO, Gabriel Henrique Campos. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models. The Astrophysical Journal, Philadelphia, v. 838, n. 2, p. 1-9, 2017. Disponível em: < http://dx.doi.org/10.3847/1538-4357/aa6002 > DOI: 10.3847/1538-4357/aa6002.
    • APA

      Caproni, A., Kowal, G., Falceta Gonçalves, D. A., Lanfranchi, G. A., & Baio, G. H. C. (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, Kowal G, Falceta Gonçalves DA, Lanfranchi GA, Baio GHC. Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models [Internet]. The Astrophysical Journal. 2017 ; 838( 2): 1-9.Available from: http://dx.doi.org/10.3847/1538-4357/aa6002
    • Vancouver

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

    Subjects: TURBULÊNCIA, MAGNETOHIDRODINÂMICA

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      KOWAL, Grzegorz; FALCETA GONÇALVES, Diego Antonio; LAZARIAN, Alex; VISHNIAC, Ethan T. Statistics of reconnection-driven turbulence. The Astrophysical Journal, Philadelphia, v. 838, n. 2, p. 1-13, 2017. Disponível em: < http://dx.doi.org/10.3847/1538-4357/aa6001 > DOI: 10.3847/1538-4357/aa6001.
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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.Available from: http://dx.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.Available from: http://dx.doi.org/10.3847/1538-4357/aa6001
  • Source: The Astrophysical Journal. Unidade: IAG

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

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      BEERS, Timothy C; PLACCO, Vinicius M; CAROLLO, Daniela; et al. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, Chicago, v. 835, p. 81, 2017. Disponível em: < http://iopscience.iop.org/article/10.3847/1538-4357/835/1/81/pdf > DOI: 10.3847/1538-4357/835/1/81.
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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
    • NLM

      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.Available from: http://iopscience.iop.org/article/10.3847/1538-4357/835/1/81/pdf
    • 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.Available from: http://iopscience.iop.org/article/10.3847/1538-4357/835/1/81/pdf

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