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  • 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://iopscience.iop.org/article/10.3847/1538-4357/ab6f76/pdf. Acesso em: 04 dez. 2022.
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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
    • NLM

      Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2022 dez. 04 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab6f76/pdf
    • 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 2022 dez. 04 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab6f76/pdf
  • 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] 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 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: 04 dez. 2022.
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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
    • NLM

      Michtchenko TA, Barros DA, Perez-Villegas A, Lépine JRD. Moving Groups as the Origin of the Vertical Phase-space Spiral in the Galactic Neighborhood [Internet]. The Astrophysical Journal. 2019 ; 876( 1): 36/1-36/7.[citado 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: https://doi.org/10.3847/1538-4357/ab11cd
  • 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: 04 dez. 2022.
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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.[citado 2022 dez. 04 ] 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 2022 dez. 04 ] 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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    • ABNT

      SILVA, Leandro Beraldo e et al. The discreteness-driven relaxation of collisionless gravitating systems: entropy evolution in external potentials, n-dependence and the role of chaos. The Astrophysical Journal, v. 870, n. 2, p. 128, 2019Tradução . . Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/aaf397/pdf. Acesso em: 04 dez. 2022.
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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.[citado 2022 dez. 04 ] 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.[citado 2022 dez. 04 ] 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. 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: http://dx.doi.org/10.3847/1538-4357/ab2460. Acesso em: 04 dez. 2022.
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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
    • NLM

      Páez A, Jatenco-Pereira V, Gonçalves DAF, Opher M. Corrugated features in coronal-mass-ejection-driven shocks: a discussion on the predisposition to particle acceleration [Internet]. The Astrophysical Journal. 2019 ; 879( 2): 01-09.[citado 2022 dez. 04 ] Available from: http://dx.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 2022 dez. 04 ] 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 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: 04 dez. 2022.
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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
    • NLM

      Guerrero G, Zaire B, Smolarkiewicz PK, Dal Pino EM de G, Kosovichev AG, Mansour NN. What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars? [Internet]. The Astrophysical Journal. 2019 ; 880( 1): 6/1-6/20.[citado 2022 dez. 04 ] 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 2022 dez. 04 ] 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 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: 04 dez. 2022.
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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
    • NLM

      Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
  • 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aaa3fc/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subject: 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: 04 dez. 2022.
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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, 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.[citado 2022 dez. 04 ] 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.[citado 2022 dez. 04 ] Available from: https://doi.org/10.3847/1538-4357/aaa1ec
  • Source: The Astrophysical Journal. Unidade: IAG

    Subject: 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] 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 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: 04 dez. 2022.
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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.[citado 2022 dez. 04 ] 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 2022 dez. 04 ] 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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      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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: https://doi.org/10.3847/1538-4357/aa6347
  • 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 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: http://iopscience.iop.org/article/10.3847/1538-4357/835/1/81/pdf. Acesso em: 04 dez. 2022.
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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 2022 dez. 04 ] 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.[citado 2022 dez. 04 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/835/1/81/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/824/1/48/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/819/2/131/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: http://iopscience.iop.org.ez67.periodicos.capes.gov.br/article/10.3847/0004-637X/825/1/54/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subject: 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: 04 dez. 2022.
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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 2022 dez. 04 ] 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 2022 dez. 04 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/830/2/57/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subject: ASTROFÍSICA ESTELAR

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      SILAJ, j e JONES, C. E e CARCIOFI, Alex Cavaliéri. Investigating the circumstellar disk of the Be shell star 48 librae. The Astrophysical Journal, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf. Acesso em: 04 dez. 2022.
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      Silaj, j, Jones, C. E., & Carciofi, A. C. (2016). Investigating the circumstellar disk of the Be shell star 48 librae. The Astrophysical Journal. doi:10.3847/0004-637X/826/1/81
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      Silaj j, Jones CE, Carciofi AC. Investigating the circumstellar disk of the Be shell star 48 librae [Internet]. The Astrophysical Journal. 2016 ;[citado 2022 dez. 04 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf
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      Silaj j, Jones CE, Carciofi AC. Investigating the circumstellar disk of the Be shell star 48 librae [Internet]. The Astrophysical Journal. 2016 ;[citado 2022 dez. 04 ] Available from: http://iopscience.iop.org/article/10.3847/0004-637X/826/81/pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: POEIRA INTERESTELAR, MEIO INTERESTELAR, CAMPO MAGNÉTICO, POLARIZAÇÃO (ASTRONOMIA), SOL

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      FRISCH, P. C et al. Evidence for an interstellar dust filament in the outer heliosheath. The Astrophysical Journal, v. 805, p. 60/1-60/8, 2015Tradução . . Disponível em: http://dx.doi.org/10.1088/0004-637X/805/1/60. Acesso em: 04 dez. 2022.
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      Frisch, P. C., Andersson, B. -G., Berdyugin, A., Piirola, V., Funsten, H. O., Magalhães, A. M., et al. (2015). Evidence for an interstellar dust filament in the outer heliosheath. The Astrophysical Journal, 805, 60/1-60/8. doi:10.1088/0004-637X/805/1/60
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      Frisch PC, Andersson B-G, Berdyugin A, Piirola V, Funsten HO, Magalhães AM, Seriacopi DB, McComas DJ, Schwadron NA, Slavin JD, Wiktorowicz SJ. Evidence for an interstellar dust filament in the outer heliosheath [Internet]. The Astrophysical Journal. 2015 ; 805 60/1-60/8.[citado 2022 dez. 04 ] Available from: http://dx.doi.org/10.1088/0004-637X/805/1/60
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      Frisch PC, Andersson B-G, Berdyugin A, Piirola V, Funsten HO, Magalhães AM, Seriacopi DB, McComas DJ, Schwadron NA, Slavin JD, Wiktorowicz SJ. Evidence for an interstellar dust filament in the outer heliosheath [Internet]. The Astrophysical Journal. 2015 ; 805 60/1-60/8.[citado 2022 dez. 04 ] Available from: http://dx.doi.org/10.1088/0004-637X/805/1/60

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