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  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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    • ABNT

      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://doi.org/10.3847/1538-4357/aad37d. Acesso em: 16 out. 2024.
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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 2024 out. 16 ] Available from: https://doi.org/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 2024 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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    • ABNT

      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://doi.org/10.3847/1538-4357/aad37d1a. Acesso em: 16 out. 2024.
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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 2024 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
    • 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 2024 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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    • ABNT

      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: 16 out. 2024.
    • APA

      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 2024 out. 16 ] 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 2024 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESPECTROSCOPIA

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      KNOWLES, Adam T et al. Stellar spectral models compared with empirical data. Monthly Notices of the Royal Astronomical Society, v. 486, n. 2, p. 1814-1832, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz754. Acesso em: 16 out. 2024.
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      Knowles, A. T., Sansom, A. E., Coelho, P. R. T., Prieto, C. A., Conroy, C., & Vazdekis, A. (2019). Stellar spectral models compared with empirical data. Monthly Notices of the Royal Astronomical Society, 486( 2), 1814-1832. doi:10.1093/mnras/stz754
    • NLM

      Knowles AT, Sansom AE, Coelho PRT, Prieto CA, Conroy C, Vazdekis A. Stellar spectral models compared with empirical data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 2): 1814-1832.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stz754
    • Vancouver

      Knowles AT, Sansom AE, Coelho PRT, Prieto CA, Conroy C, Vazdekis A. Stellar spectral models compared with empirical data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 2): 1814-1832.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stz754
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROQUÍMICA, ABUNDÂNCIA ESTELAR, JATOS (ASTRONOMIA)

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      DURONEA, N. U et al. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103. Monthly Notices of the Royal Astronomical Society, v. 489, n. 2, p. 1519-1532, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2087. Acesso em: 16 out. 2024.
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      Duronea, N. U., Bronfman, L., Mendoza, E., Merello, M., Finger, R., Reyes, N., et al. (2019). Cyanoacetylene in the outflow/hot molecular core G331.512-0.103. Monthly Notices of the Royal Astronomical Society, 489( 2), 1519-1532. doi:10.1093/mnras/stz2087
    • NLM

      Duronea NU, Bronfman L, Mendoza E, Merello M, Finger R, Reyes N, Hervias-Caimapo C, Faure A, Cappa CE, Arnal EM, Lépine JRD, Kleiner I, Nyman L-A. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 1519-1532.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stz2087
    • Vancouver

      Duronea NU, Bronfman L, Mendoza E, Merello M, Finger R, Reyes N, Hervias-Caimapo C, Faure A, Cappa CE, Arnal EM, Lépine JRD, Kleiner I, Nyman L-A. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 1519-1532.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stz2087
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS VARIÁVEIS, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      KOVTYUKH, V. V et al. Elemental abundances in the centre of the Galactic nuclear disc. Monthly Notices of the Royal Astronomical Society, v. 489, n. 2, p. 2254-2260, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2316. Acesso em: 16 out. 2024.
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      Kovtyukh, V. V., Andrievsky, S. M., Martin, R. P., Korotin, S. A., Lépine, J. R. D., Maciel, W. J., et al. (2019). Elemental abundances in the centre of the Galactic nuclear disc. Monthly Notices of the Royal Astronomical Society, 489( 2), 2254-2260. doi:10.1093/mnras/stz2316
    • NLM

      Kovtyukh VV, Andrievsky SM, Martin RP, Korotin SA, Lépine JRD, Maciel WJ, Keir LE, Panko EA. Elemental abundances in the centre of the Galactic nuclear disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 2254-2260.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stz2316
    • Vancouver

      Kovtyukh VV, Andrievsky SM, Martin RP, Korotin SA, Lépine JRD, Maciel WJ, Keir LE, Panko EA. Elemental abundances in the centre of the Galactic nuclear disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 2254-2260.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stz2316
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS BINARIAS

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      RAMIREZ, et al. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 16 out. 2024.
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      Ramirez,, Khanal, S., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/sty104
    • NLM

      Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 out. 16 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 out. 16 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES

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      LAGIOIA, E. P et al. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, v. 475, n. 3, p. 4088-4103, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty083. Acesso em: 16 out. 2024.
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      Lagioia, E. P., Milone, A. P., Marino, A. F., Cassisi, S., Aparicio, A. J., Piotto, G., et al. (2018). The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, 475( 3), 4088-4103. doi:10.1093/mnras/sty083
    • NLM

      Lagioia EP, Milone AP, Marino AF, Cassisi S, Aparicio AJ, Piotto G, Anderson J, Barbuy BLS. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 4088-4103.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/sty083
    • Vancouver

      Lagioia EP, Milone AP, Marino AF, Cassisi S, Aparicio AJ, Piotto G, Anderson J, Barbuy BLS. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 4088-4103.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/sty083
  • Source: Astronomical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESPECTROSCOPIA

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      PLACCO, Vinicius M et al. Spectroscopic validation of low-metallicity stars from RAVE. Astronomical Journal, v. 155, n. 6, p. 256, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-3881/aac20c. Acesso em: 16 out. 2024.
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      Placco, V. M., Beers, J., Santucci, R. M., Chanamé, J., & Rossi, S. C. F. (2018). Spectroscopic validation of low-metallicity stars from RAVE. Astronomical Journal, 155( 6), 256. doi:10.3847/1538-3881/aac20c
    • NLM

      Placco VM, Beers J, Santucci RM, Chanamé J, Rossi SCF. Spectroscopic validation of low-metallicity stars from RAVE [Internet]. Astronomical Journal. 2018 ; 155( 6): 256.[citado 2024 out. 16 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
    • Vancouver

      Placco VM, Beers J, Santucci RM, Chanamé J, Rossi SCF. Spectroscopic validation of low-metallicity stars from RAVE [Internet]. Astronomical Journal. 2018 ; 155( 6): 256.[citado 2024 out. 16 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
  • 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: 16 out. 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 out. 16 ] 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 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aad908
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: DISCOS DE ACRESÇÃO, ABUNDÂNCIA ESTELAR

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      TAKEDA, L et al. 3D photoionization models of nova V723 Cas. Monthly Notices of the Royal Astronomical Society, v. 473, n. 1, p. 355-365, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2285. Acesso em: 16 out. 2024.
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      Takeda, L., Diaz, M. P., Campbell, R., & Lyke, J. (2018). 3D photoionization models of nova V723 Cas. Monthly Notices of the Royal Astronomical Society, 473( 1), 355-365. doi:10.1093/mnras/stx2285
    • NLM

      Takeda L, Diaz MP, Campbell R, Lyke J. 3D photoionization models of nova V723 Cas [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 473( 1): 355-365.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stx2285
    • Vancouver

      Takeda L, Diaz MP, Campbell R, Lyke J. 3D photoionization models of nova V723 Cas [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 473( 1): 355-365.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stx2285
  • 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: 16 out. 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
    • 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 2024 out. 16 ] 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 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
  • 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: 16 out. 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
    • 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 2024 out. 16 ] 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 out. 16 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      LIU, F et al. The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, v. 457, p. 3934-3948, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw247. Acesso em: 16 out. 2024.
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      Liu, F., Yong, D., Asplund, M., Ramírez, I., & Moreno, J. L. M. (2016). The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, 457, 3934-3948. doi:10.1093/mnras/stw247
    • NLM

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw247
    • Vancouver

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw247
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      ANDRIEVSKY, S. M et al. Oxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc - II. Monthly Notices of the Royal Astronomical Society, v. 461, p. 4256-4259, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw1631. Acesso em: 16 out. 2024.
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      Andrievsky, S. M., Martin, R. P., Kovtyukh, V. V., Korotin, S. A., & Lépine, J. R. D. (2016). Oxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc - II. Monthly Notices of the Royal Astronomical Society, 461, 4256-4259. doi:10.1093/mnras/stw1631
    • NLM

      Andrievsky SM, Martin RP, Kovtyukh VV, Korotin SA, Lépine JRD. Oxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc - II [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 461 4256-4259.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw1631
    • Vancouver

      Andrievsky SM, Martin RP, Kovtyukh VV, Korotin SA, Lépine JRD. Oxygen, α-element and iron abundance distributions in the inner part of the Galactic thin disc - II [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 461 4256-4259.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw1631
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      LIU, F et al. The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2636-2646, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2821. Acesso em: 16 out. 2024.
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      Liu, F., Yong, D., Asplund, M., Ramírez, I., Moreno, J. L. M., Gustafsson, B., et al. (2016). The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, 456, 2636-2646. doi:10.1093/mnras/stv2821
    • NLM

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stv2821
    • Vancouver

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stv2821
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR

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      PLACCO, Vinicius M et al. G64-12 and G64-37 are carbon-enhanced metal-poor stars. The Astrophysical Journal Letters, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf. Acesso em: 16 out. 2024.
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      Placco, V. M., Beers, T. C., Reggiani, H., & Moreno, J. L. M. (2016). G64-12 and G64-37 are carbon-enhanced metal-poor stars. The Astrophysical Journal Letters. doi:10.3847/2041-8205/829/2/L24
    • NLM

      Placco VM, Beers TC, Reggiani H, Moreno JLM. G64-12 and G64-37 are carbon-enhanced metal-poor stars [Internet]. The Astrophysical Journal Letters. 2016 ;[citado 2024 out. 16 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
    • Vancouver

      Placco VM, Beers TC, Reggiani H, Moreno JLM. G64-12 and G64-37 are carbon-enhanced metal-poor stars [Internet]. The Astrophysical Journal Letters. 2016 ;[citado 2024 out. 16 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR

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      YONG, David et al. GRACES observations of young [α/Fe]-rich stars. Monthly Notices of the Royal Astronomical Society, v. 459, p. 487-495, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw676. Acesso em: 16 out. 2024.
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      Yong, D., Casagrande, L., Venn, K. A., Chené, A. -N., Keown, J., Malo, L., et al. (2016). GRACES observations of young [α/Fe]-rich stars. Monthly Notices of the Royal Astronomical Society, 459, 487-495. doi:10.1093/mnras/stw676
    • NLM

      Yong D, Casagrande L, Venn KA, Chené A-N, Keown J, Malo L, Martioli E, Moreno JLM. GRACES observations of young [α/Fe]-rich stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 459 487-495.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw676
    • Vancouver

      Yong D, Casagrande L, Venn KA, Chené A-N, Keown J, Malo L, Martioli E, Moreno JLM. GRACES observations of young [α/Fe]-rich stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 459 487-495.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw676
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      ASPLUND, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, v. 463, p. 696-704, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 16 out. 2024.
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      Asplund, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 463, 696-704. doi:10.1093/mnras/stw2045
    • NLM

      Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw2045
    • Vancouver

      Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw2045
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: ABUNDÂNCIA ESTELAR

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      LIU, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 16 out. 2024.
    • APA

      Liu, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stw2045
    • NLM

      Liu F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw2045
    • Vancouver

      Liu F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2024 out. 16 ] Available from: https://doi.org/10.1093/mnras/stw2045

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