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  • Source: Astrophysical Journal. Unidades: IAG, EACH, IF

    Subjects: ASTROFÍSICA, MAGNETOHIDRODINÂMICA, RAIOS CÓSMICOS, ACELERAÇÃO DE PARTÍCULAS, NEUTRINOS

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    • ABNT

      MEDINA-TORREJON, Tania et al. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets. Astrophysical Journal, v. 908, n. 2, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abd6c2. Acesso em: 02 dez. 2022.
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      Medina-Torrejon, T., Dal Pino, E. de G., Kadowaki, L. H. S., Kowal, G., Singh, C. B., & Mizuno, Y. (2021). Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets. Astrophysical Journal, 908( 2). doi:10.3847/1538-4357/abd6c2
    • NLM

      Medina-Torrejon T, Dal Pino E de G, Kadowaki LHS, Kowal G, Singh CB, Mizuno Y. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets [Internet]. Astrophysical Journal. 2021 ; 908( 2):[citado 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/abd6c2
    • Vancouver

      Medina-Torrejon T, Dal Pino E de G, Kadowaki LHS, Kowal G, Singh CB, Mizuno Y. Particle Acceleration by Relativistic Magnetic Reconnection Driven by Kink Instability Turbulence in Poynting Flux–Dominated Jets [Internet]. Astrophysical Journal. 2021 ; 908( 2):[citado 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/abd6c2
  • Source: Astrophysical Journal. Unidades: IAG, IF

    Subjects: ASTROFÍSICA, RELATIVIDADE (FÍSICA), MAGNETOHIDRODINÂMICA, ACELERAÇÃO DE PARTÍCULAS, JATOS (ASTRONOMIA)

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    • ABNT

      KADOWAKI, Luis H. S. et al. Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets. Astrophysical Journal, v. 912, n. 2, 2021Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abee7a. Acesso em: 02 dez. 2022.
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      Kadowaki, L. H. S., Dal Pino, E. de G., Torrejón, T. M., Mizuno, Y., & Kushwaha, P. (2021). Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets. Astrophysical Journal, 912( 2). doi:10.3847/1538-4357/abee7a
    • NLM

      Kadowaki LHS, Dal Pino E de G, Torrejón TM, Mizuno Y, Kushwaha P. Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets [Internet]. Astrophysical Journal. 2021 ; 912( 2):[citado 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/abee7a
    • Vancouver

      Kadowaki LHS, Dal Pino E de G, Torrejón TM, Mizuno Y, Kushwaha P. Fast Magnetic Reconnection Structures in Poynting Flux-dominated Jets [Internet]. Astrophysical Journal. 2021 ; 912( 2):[citado 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/abee7a
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      NASCIMENTO J.-D. DO, et al. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, v. 898, p. 173 2020, 2020Tradução . . Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/ab9c16/pdf. Acesso em: 02 dez. 2022.
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      Nascimento J.-D. do,, Almeida, L. de, Velloso, E. N., Anthony, F., Costa, J. S. da, Castro, M., & Moreno, J. L. M. (2020). Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, 898, 173 2020. doi:10.3847/1538-4357/ab9c16
    • NLM

      Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9c16/pdf
    • Vancouver

      Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9c16/pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      CAIN, Madelyn e MORENO, Jorge Luis Meléndez. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, v. 864, p. 43 2020, 2020Tradução . . Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/aad37d. Acesso em: 02 dez. 2022.
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      Cain, M., & Moreno, J. L. M. (2020). The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, 864, 43 2020. doi:10.3847/1538-4357/aad37d
    • NLM

      Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/aad37d
    • Vancouver

      Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/aad37d
  • Source: Astrophysical Journal. Unidade: IAG

    Subject: GALÁXIAS

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      GARCIA, A. e HORVATH, Jorge Ernesto. A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g. Astrophysical Journal, v. 903p. 75 2020, 2020Tradução . . Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/abb823/pdf. Acesso em: 02 dez. 2022.
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      Garcia, A., & Horvath, J. E. (2020). A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g. Astrophysical Journal, 903p. 75 2020. doi:10.3847/1538-4357/abb823
    • NLM

      Garcia A, Horvath JE. A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g [Internet]. Astrophysical Journal. 2020 ; 903p. 75 2020[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/abb823/pdf
    • Vancouver

      Garcia A, Horvath JE. A DESGW Search for the eectromagnetic counterpart to the LIGO/Virgo gravitational-wave binary neutron star merger candidate S190510g [Internet]. Astrophysical Journal. 2020 ; 903p. 75 2020[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/abb823/pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: TRANSFERÊNCIA RADIATIVA, ESTRELAS BINÁRIAS

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      SUFFAK, M W et al. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018. Astrophysical Journal, v. 890, 2020Tradução . . Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/ab68dc/pdf. Acesso em: 02 dez. 2022.
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      Suffak, M. W., Richardson, N. D., Jones, C. E., Tycner, C., Henry, G. W., Carciofi, A. C., et al. (2020). The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018. Astrophysical Journal, 890. doi:10.3847/1538-4357/ab68dc
    • NLM

      Suffak MW, Richardson ND, Jones CE, Tycner C, Henry GW, Carciofi AC, Mota BC, Rubio AC. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 [Internet]. Astrophysical Journal. 2020 ;890[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab68dc/pdf
    • Vancouver

      Suffak MW, Richardson ND, Jones CE, Tycner C, Henry GW, Carciofi AC, Mota BC, Rubio AC. The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018 [Internet]. Astrophysical Journal. 2020 ;890[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab68dc/pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      EZZEDDINE, Rana e MORENO, Jorge Luis Meléndez. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, v. 898, p. 150 2020, 2020Tradução . . Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/ab9d1a/pdf. Acesso em: 02 dez. 2022.
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      Ezzeddine, R., & Moreno, J. L. M. (2020). The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, 898, 150 2020. doi:10.3847/1538-4357/aad37d1a
    • NLM

      Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9d1a/pdf
    • Vancouver

      Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9d1a/pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      PLACCO, Vinicius M e SANTUCCI, Rafael M e ROSSI, Silvia Cristina Fernandes. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, v. 870, n. 2, p. 122-1/122-11, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf3b9. Acesso em: 02 dez. 2022.
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      Placco, V. M., Santucci, R. M., & Rossi, S. C. F. (2019). The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, 870( 2), 122-1/122-11. doi:10.3847/1538-4357/aaf3b9
    • NLM

      Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
    • Vancouver

      Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ASTROMETRIA, ESTRELAS BINÁRIAS

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      GALLI, Phillip A. B et al. The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region. Astrophysical Journal, v. 859, p. 33, 2018Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/1538-4357/aabf91/pdf. Acesso em: 02 dez. 2022.
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      Galli, P. A. B., Loinard, L., Otiz-Leon, G. N., & Teixeira, R. (2018). The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region. Astrophysical Journal, 859, 33. doi:10.3847/1538-4357/aabf91
    • NLM

      Galli PAB, Loinard L, Otiz-Leon GN, Teixeira R. The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region [Internet]. Astrophysical Journal. 2018 ; 859 33.[citado 2022 dez. 02 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aabf91/pdf
    • Vancouver

      Galli PAB, Loinard L, Otiz-Leon GN, Teixeira R. The Gouldʼs Belt Distances Survey (GOBELINS). IV. Distance, Depth, and Kinematics of the Taurus Star-forming Region [Internet]. Astrophysical Journal. 2018 ; 859 33.[citado 2022 dez. 02 ] Available from: http://iopscience.iop.org/article/10.3847/1538-4357/aabf91/pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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    • ABNT

      SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e GALARZA, Jhon J. Yana. How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: http://doi.org/ 10.3847/1538-4357/ab8bd7. Acesso em: 02 dez. 2022.
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      Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2018). How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/ab8bd7
    • NLM

      Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2022 dez. 02 ] Available from: http://doi.org/ 10.3847/1538-4357/ab8bd7
    • Vancouver

      Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2022 dez. 02 ] Available from: http://doi.org/ 10.3847/1538-4357/ab8bd7
  • 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: http://doi.org/10.3847/1538-4357/aad190. Acesso em: 02 dez. 2022.
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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 2022 dez. 02 ] Available from: http://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 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad190
  • Source: Astrophysical Journal. Unidade: IAG

    Subject: 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://iopscience.iop.org/article/10.3847/1538-4357/aae843. Acesso em: 02 dez. 2022.
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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
    • NLM

      Menezes RB, Steiner JE. Double nuclei in NGC 908 and NGC 1187 [Internet]. Astrophysical Journal. 2018 ; 868 67.[citado 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/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 2022 dez. 02 ] Available from: https://iopscience.iop.org/article/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: http://doi.org/10.3847/1538-4357/aad964. Acesso em: 02 dez. 2022.
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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 2022 dez. 02 ] Available from: http://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 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad964
  • 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: http://doi.org/10.3847/1538-4357/aad908. Acesso em: 02 dez. 2022.
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      Bedell, M., Casagrande, L., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., 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, Casagrande L, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad908
    • Vancouver

      Bedell M, Casagrande L, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad908
  • 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: http://doi.org/10.3847/1538-4357/aab36c. Acesso em: 02 dez. 2022.
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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
    • NLM

      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 2022 dez. 02 ] Available from: http://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 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aab36c
  • 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: http://doi.org/10.3847/1538-4357/aad4ff. Acesso em: 02 dez. 2022.
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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
    • NLM

      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 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad4ff
    • Vancouver

      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 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad4ff
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES

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    • ABNT

      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: http://doi.org/10.3847/1538-4357/aad37d. Acesso em: 02 dez. 2022.
    • APA

      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
    • NLM

      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 2022 dez. 02 ] Available from: http://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 2022 dez. 02 ] Available from: http://doi.org/10.3847/1538-4357/aad37d
  • Source: Astrophysical Journal. Unidade: IAG

    Subject: GALÁXIAS

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    • ABNT

      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: 02 dez. 2022.
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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/aa8ef5
    • NLM

      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 2022 dez. 02 ] 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 2022 dez. 02 ] 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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    • ABNT

      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: 02 dez. 2022.
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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
    • NLM

      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 2022 dez. 02 ] 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 2022 dez. 02 ] Available from: https://arxiv.org/pdf/1710.05031.pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR

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    • ABNT

      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: 02 dez. 2022.
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      Dulaney, N. A., Gerhartz, C. J., Carciofi, A. C., & Richardson, N. D. (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
    • NLM

      Dulaney NA, Gerhartz CJ, Carciofi AC, Richardson ND. A Spectroscopic Orbit for the late-type Be star β CMi [Internet]. Astrophysical Journal. 2017 ;836( 1): 112.[citado 2022 dez. 02 ] Available from: https://arxiv.org/abs/1701.05201
    • Vancouver

      Dulaney NA, Gerhartz CJ, Carciofi AC, Richardson ND. A Spectroscopic Orbit for the late-type Be star β CMi [Internet]. Astrophysical Journal. 2017 ;836( 1): 112.[citado 2022 dez. 02 ] Available from: https://arxiv.org/abs/1701.05201

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