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  • Source: Astrophysical Journal. Unidade: IF

    Subjects: GALÁXIAS, CLUSTERS, MATÉRIA ESCURA

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      RUMBAUGH, N. e LIMA, Marcos Vinicius Borges Teixeira. Extreme variability quasars from the sloan digital sky survey and the dark energy survey. Astrophysical Journal, v. fe 2018, n. 2, p. 160, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaa9b6. Acesso em: 23 abr. 2024.
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      Rumbaugh, N., & Lima, M. V. B. T. (2018). Extreme variability quasars from the sloan digital sky survey and the dark energy survey. Astrophysical Journal, fe 2018( 2), 160. doi:10.3847/1538-4357/aaa9b6
    • NLM

      Rumbaugh N, Lima MVBT. Extreme variability quasars from the sloan digital sky survey and the dark energy survey [Internet]. Astrophysical Journal. 2018 ; fe 2018( 2): 160.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aaa9b6
    • Vancouver

      Rumbaugh N, Lima MVBT. Extreme variability quasars from the sloan digital sky survey and the dark energy survey [Internet]. Astrophysical Journal. 2018 ; fe 2018( 2): 160.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aaa9b6
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      SPINA, Lorenzo et al. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, v. 863, n. 2, p. 179-1/179-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 23 abr. 2024.
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      Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
    • NLM

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad190
    • Vancouver

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad190
  • Source: Astrophysical Journal. Unidade: IF

    Subjects: GALÁXIAS, CLUSTERS, MATÉRIA ESCURA

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      CHANG, C. e LIMA, Marcos Vinicius Borges Teixeira. The splashback feature around DES galaxy clusters: galaxy density and weak lensing profiles. Astrophysical Journal, v. 864, n. 1, p. 83, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad5e7. Acesso em: 23 abr. 2024.
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      Chang, C., & Lima, M. V. B. T. (2018). The splashback feature around DES galaxy clusters: galaxy density and weak lensing profiles. Astrophysical Journal, 864( 1), 83. doi:10.3847/1538-4357/aad5e7
    • NLM

      Chang C, Lima MVBT. The splashback feature around DES galaxy clusters: galaxy density and weak lensing profiles [Internet]. Astrophysical Journal. 2018 ; 864( 1): 83.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad5e7
    • Vancouver

      Chang C, Lima MVBT. The splashback feature around DES galaxy clusters: galaxy density and weak lensing profiles [Internet]. Astrophysical Journal. 2018 ; 864( 1): 83.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad5e7
  • Source: Astrophysical Journal. Unidade: IF

    Subjects: REAÇÕES NUCLEARES, FÍSICA NUCLEAR, ASTROFÍSICA NUCLEAR

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      LAU, R. et al. Nuclear reactions in the crusts of accreting neutron stars. Astrophysical Journal, v. 859, n. 1, p. 62, 2018Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/1538-4357/aabfe0/meta. Acesso em: 23 abr. 2024.
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      Lau, R., Beard, M., Gupta, S. S., Schatz, H., Afanasjev, A. V., Brown, E. F., et al. (2018). Nuclear reactions in the crusts of accreting neutron stars. Astrophysical Journal, 859( 1), 62. doi:10.3847/1538-4357/aabfe0
    • NLM

      Lau R, Beard M, Gupta SS, Schatz H, Afanasjev AV, Brown EF, Deibel A, Hitt GW, Hix WR, Keek L, Moller P, Shternin PS, Steiner AW, Wiescher M, Xu Y, Gasques LR. Nuclear reactions in the crusts of accreting neutron stars [Internet]. Astrophysical Journal. 2018 ; 859( 1): 62.[citado 2024 abr. 23 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aabfe0/meta
    • Vancouver

      Lau R, Beard M, Gupta SS, Schatz H, Afanasjev AV, Brown EF, Deibel A, Hitt GW, Hix WR, Keek L, Moller P, Shternin PS, Steiner AW, Wiescher M, Xu Y, Gasques LR. Nuclear reactions in the crusts of accreting neutron stars [Internet]. Astrophysical Journal. 2018 ; 859( 1): 62.[citado 2024 abr. 23 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aabfe0/meta
  • Source: Astrophysical Journal. Unidades: IF, EEL, IFSC

    Subjects: RAIOS CÓSMICOS, ASTROFÍSICA, OBSERVATÓRIOS

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      AAB, A. et al. Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger pbservatory. Astrophysical Journal, v. No 2018, n. 1, p. 4-1-4-12, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aae689. Acesso em: 23 abr. 2024.
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      Aab, A., Albuquerque, I. F. da M. e, Catalani, F., Souza, V. de, Kemmerich, N., Lang, R. G., et al. (2018). Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger pbservatory. Astrophysical Journal, No 2018( 1), 4-1-4-12. doi:10.3847/1538-4357/aae689
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      Aab A, Albuquerque IF da M e, Catalani F, Souza V de, Kemmerich N, Lang RG, Prado RR, Carvalho WR de, Santos EM, Peixoto CJT. Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger pbservatory [Internet]. Astrophysical Journal. 2018 ; No 2018( 1): 4-1-4-12.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aae689
    • Vancouver

      Aab A, Albuquerque IF da M e, Catalani F, Souza V de, Kemmerich N, Lang RG, Prado RR, Carvalho WR de, Santos EM, Peixoto CJT. Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger pbservatory [Internet]. Astrophysical Journal. 2018 ; No 2018( 1): 4-1-4-12.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aae689
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

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      BEDELL, Megan et al. The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, v. 865, n. 1, p. 68-1/68-13, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad908. Acesso em: 23 abr. 2024.
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      Bedell, M., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., Asplund, M., et al. (2018). The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, 865( 1), 68-1/68-13. doi:10.3847/1538-4357/aad908
    • NLM

      Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad908
    • Vancouver

      Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad908
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: GALÁXIAS

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      MENEZES, R. B e STEINER, João Evangelista. Double nuclei in NGC 908 and NGC 1187. Astrophysical Journal, v. 868, p. 67, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aae843. Acesso em: 23 abr. 2024.
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      Menezes, R. B., & Steiner, J. E. (2018). Double nuclei in NGC 908 and NGC 1187. Astrophysical Journal, 868, 67. doi:10.3847/1538-4357/aae843
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      Menezes RB, Steiner JE. Double nuclei in NGC 908 and NGC 1187 [Internet]. Astrophysical Journal. 2018 ; 868 67.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aae843
    • Vancouver

      Menezes RB, Steiner JE. Double nuclei in NGC 908 and NGC 1187 [Internet]. Astrophysical Journal. 2018 ; 868 67.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aae843
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR

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      CHOJNOWSKI, S. Drew et al. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, v. 865, n. 1, p. 76-1/76-16, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad964. Acesso em: 23 abr. 2024.
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      Chojnowski, S. D., Labadie-Bartz, J., Rivinius, T., Gies, D., & Leister, N. V. (2018). The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, 865( 1), 76-1/76-16. doi:10.3847/1538-4357/aad964
    • NLM

      Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad964
    • Vancouver

      Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad964
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      CARLOS, Marília et al. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 23 abr. 2024.
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      Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
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      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
    • Vancouver

      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
  • Source: Astrophysical Journal. Unidade: IF

    Subjects: GALÁXIAS, CLUSTERS, MATÉRIA ESCURA

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      SMITH, M. e LIMA, Marcos Vinicius Borges Teixeira. Studying the ultraviolet spectrum of the first spectroscopically confirmed supernova at redshift two. Astrophysical Journal, v. fe 2018, n. 1, p. 37, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaa126. Acesso em: 23 abr. 2024.
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      Smith, M., & Lima, M. V. B. T. (2018). Studying the ultraviolet spectrum of the first spectroscopically confirmed supernova at redshift two. Astrophysical Journal, fe 2018( 1), 37. doi:10.3847/1538-4357/aaa126
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      Smith M, Lima MVBT. Studying the ultraviolet spectrum of the first spectroscopically confirmed supernova at redshift two [Internet]. Astrophysical Journal. 2018 ; fe 2018( 1): 37.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aaa126
    • Vancouver

      Smith M, Lima MVBT. Studying the ultraviolet spectrum of the first spectroscopically confirmed supernova at redshift two [Internet]. Astrophysical Journal. 2018 ; fe 2018( 1): 37.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aaa126
  • Source: Astrophysical Journal. Unidade: IF

    Subjects: GALÁXIAS, CLUSTERS, MATÉRIA ESCURA

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      AGUIRRE, Paula e LIMA, Marcos Vinicius Borges Teixeira. The LABOCA/ACT survey of clusters at all redshifts: multiwavelength analysis of background submillimeter galaxies. Astrophysical Journal, v. 851, n. 1, p. 26, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaaab0. Acesso em: 23 abr. 2024.
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      Aguirre, P., & Lima, M. V. B. T. (2018). The LABOCA/ACT survey of clusters at all redshifts: multiwavelength analysis of background submillimeter galaxies. Astrophysical Journal, 851( 1), 26. doi:10.3847/1538-4357/aaaab0
    • NLM

      Aguirre P, Lima MVBT. The LABOCA/ACT survey of clusters at all redshifts: multiwavelength analysis of background submillimeter galaxies [Internet]. Astrophysical Journal. 2018 ; 851( 1): 26.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aaaab0
    • Vancouver

      Aguirre P, Lima MVBT. The LABOCA/ACT survey of clusters at all redshifts: multiwavelength analysis of background submillimeter galaxies [Internet]. Astrophysical Journal. 2018 ; 851( 1): 26.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aaaab0
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES

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      CAIN, Madelyn et al. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, v. 864, n. 1, p. 43-1/43-12, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 23 abr. 2024.
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      Cain, M., Frebel, A., Gull, M., Ji, A. P., Placco, V. M., Beers, T. C., et al. (2018). The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, 864( 1), 43-1/43-12. doi:10.3847/1538-4357/aad37d
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      Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
    • Vancouver

      Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: DISCOS DE ACRESÇÃO, MAGNETOHIDRODINÂMICA

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      KADOWAKI, Luis H. S e DAL PINO, Elisabete Maria de Gouveia e STONE, James M. MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection. Astrophysical Journal, v. 864, n. 1, p. 52-1/52-17, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad4ff. Acesso em: 23 abr. 2024.
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      Kadowaki, L. H. S., Dal Pino, E. M. de G., & Stone, J. M. (2018). MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection. Astrophysical Journal, 864( 1), 52-1/52-17. doi:10.3847/1538-4357/aad4ff
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      Kadowaki LHS, Dal Pino EM de G, Stone JM. MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection [Internet]. Astrophysical Journal. 2018 ; 864( 1): 52-1/52-17.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad4ff
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      Kadowaki LHS, Dal Pino EM de G, Stone JM. MHD instabilities in accretion disks and their implications in driving fast magnetic reconnection [Internet]. Astrophysical Journal. 2018 ; 864( 1): 52-1/52-17.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad4ff
  • Source: Astrophysical Journal. Unidade: IF

    Subjects: GALÁXIAS, CLUSTERS, MATÉRIA ESCURA

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      ABBOTT, T. M. C. e LIMA, Marcos Vinicius Borges Teixeira. The dark energy survey: data release 1. Astrophysical Journal, v. 239, n. 2, p. 18, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/aae9f0. Acesso em: 23 abr. 2024.
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      Abbott, T. M. C., & Lima, M. V. B. T. (2018). The dark energy survey: data release 1. Astrophysical Journal, 239( 2), 18. doi:10.3847/1538-4365/aae9f0
    • NLM

      Abbott TMC, Lima MVBT. The dark energy survey: data release 1 [Internet]. Astrophysical Journal. 2018 ; 239( 2): 18.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4365/aae9f0
    • Vancouver

      Abbott TMC, Lima MVBT. The dark energy survey: data release 1 [Internet]. Astrophysical Journal. 2018 ; 239( 2): 18.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4365/aae9f0
  • Source: Astrophysical Journal. Unidade: IAG

    Assunto: GALÁXIAS

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      SILVA, Leandro Beraldo e et al. The Arrow of Time in the Collapse of Collisionless Self-gravitating Systems: Non-validity of the Vlasov–Poisson Equation during Violent Relaxation. Astrophysical Journal, v. 846, p. 125, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa876e. Acesso em: 23 abr. 2024.
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      Silva, L. B. e, Pedra, W. de S., Sodré Júnior, L., Perico, E. L. D., & Lima, M. (2017). The Arrow of Time in the Collapse of Collisionless Self-gravitating Systems: Non-validity of the Vlasov–Poisson Equation during Violent Relaxation. Astrophysical Journal, 846, 125. doi:10.3847/1538-4357/aa876e
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      Silva LB e, Pedra W de S, Sodré Júnior L, Perico ELD, Lima M. The Arrow of Time in the Collapse of Collisionless Self-gravitating Systems: Non-validity of the Vlasov–Poisson Equation during Violent Relaxation [Internet]. Astrophysical Journal. 2017 ; 846 125.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa876e
    • Vancouver

      Silva LB e, Pedra W de S, Sodré Júnior L, Perico ELD, Lima M. The Arrow of Time in the Collapse of Collisionless Self-gravitating Systems: Non-validity of the Vlasov–Poisson Equation during Violent Relaxation [Internet]. Astrophysical Journal. 2017 ; 846 125.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa876e
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: DISCOS DE ACRESÇÃO, BURACOS NEGROS

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      WONG, Ka-Wah et al. Hard x-ray emission from the M87 AGN detected with NuSTAR. Astrophysical Journal, v. 849, p. L17, 2017Tradução . . Disponível em: https://arxiv.org/pdf/1710.05031.pdf. Acesso em: 23 abr. 2024.
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      Wong, K. -W., Silva, R. N. da, Irwin, J. A., & Lin, D. (2017). Hard x-ray emission from the M87 AGN detected with NuSTAR. Astrophysical Journal, 849, L17. doi:10.3847/2041-8213/aa92c2
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      Wong K-W, Silva RN da, Irwin JA, Lin D. Hard x-ray emission from the M87 AGN detected with NuSTAR [Internet]. Astrophysical Journal. 2017 ; 849 L17.[citado 2024 abr. 23 ] Available from: https://arxiv.org/pdf/1710.05031.pdf
    • Vancouver

      Wong K-W, Silva RN da, Irwin JA, Lin D. Hard x-ray emission from the M87 AGN detected with NuSTAR [Internet]. Astrophysical Journal. 2017 ; 849 L17.[citado 2024 abr. 23 ] Available from: https://arxiv.org/pdf/1710.05031.pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR

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      DULANEY, Nicholas A et al. A Spectroscopic Orbit for the late-type Be star β CMi. Astrophysical Journal, v. 836, n. 1, p. 112, 2017Tradução . . Disponível em: https://arxiv.org/abs/1701.05201. Acesso em: 23 abr. 2024.
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      Dulaney, N. A., Richardson, N. D., Gerhartz, C. J., & Carciofi, A. C. (2017). A Spectroscopic Orbit for the late-type Be star β CMi. Astrophysical Journal, 836( 1), 112. doi:10.3847/1538-4357/836/1/112
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      Dulaney NA, Richardson ND, Gerhartz CJ, Carciofi AC. A Spectroscopic Orbit for the late-type Be star β CMi [Internet]. Astrophysical Journal. 2017 ;836( 1): 112.[citado 2024 abr. 23 ] Available from: https://arxiv.org/abs/1701.05201
    • Vancouver

      Dulaney NA, Richardson ND, Gerhartz CJ, Carciofi AC. A Spectroscopic Orbit for the late-type Be star β CMi [Internet]. Astrophysical Journal. 2017 ;836( 1): 112.[citado 2024 abr. 23 ] Available from: https://arxiv.org/abs/1701.05201
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

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      BEDELL, Megan et al. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, v. 839, p. 94. 2017, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6a1d. Acesso em: 23 abr. 2024.
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      Bedell, M., Bean, J. L., Moreno, J. L. M., Mills, S. M., Fabrycky, D. C., Freitas, F. C., et al. (2017). Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, 839, 94. 2017. doi:10.3847/1538-4357/aa6a1d
    • NLM

      Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
    • Vancouver

      Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, SOL

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      LÉPINE, Jacques Raymond Daniel et al. The Dynamical Origin of the Local Arm and the Sunʼs Trapped Orbit. Astrophysical Journal, v. 843, p. 48, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa72e5. Acesso em: 23 abr. 2024.
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      Lépine, J. R. D., Michtchenko, T. A., Barros, D. A., & Vieira, R. S. S. (2017). The Dynamical Origin of the Local Arm and the Sunʼs Trapped Orbit. Astrophysical Journal, 843, 48. doi:10.3847/1538-4357/aa72e5
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      Lépine JRD, Michtchenko TA, Barros DA, Vieira RSS. The Dynamical Origin of the Local Arm and the Sunʼs Trapped Orbit [Internet]. Astrophysical Journal. 2017 ; 843 48.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa72e5
    • Vancouver

      Lépine JRD, Michtchenko TA, Barros DA, Vieira RSS. The Dynamical Origin of the Local Arm and the Sunʼs Trapped Orbit [Internet]. Astrophysical Journal. 2017 ; 843 48.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa72e5
  • Source: Astrophysical Journal. Unidade: IFSC

    Subjects: FÍSICA DE ALTA ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA

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      APEL, W. D. e SOUZA, Vitor de. KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100TeV and 1 EeV. Astrophysical Journal, v. 848, n. 1, p. 1-1-1-7, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa8bb7. Acesso em: 23 abr. 2024.
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      Apel, W. D., & Souza, V. de. (2017). KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100TeV and 1 EeV. Astrophysical Journal, 848( 1), 1-1-1-7. doi:10.3847/1538-4357/aa8bb7
    • NLM

      Apel WD, Souza V de. KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100TeV and 1 EeV [Internet]. Astrophysical Journal. 2017 ; 848( 1): 1-1-1-7.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa8bb7
    • Vancouver

      Apel WD, Souza V de. KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100TeV and 1 EeV [Internet]. Astrophysical Journal. 2017 ; 848( 1): 1-1-1-7.[citado 2024 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aa8bb7

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