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Filtros : "Estados Unidos" "Beers, Timothy C" "MORENO, JORGE LUIS MELENDEZ" Removidos: "Universidade de São Paulo (USP)" "EERP-ERG" Limpar

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  • Artigo de periodico

    The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild (2018)

    Cain, Madelyn; Frebel, Anna; Gull, Maude; Ji, Alexander P; Placco, Vinicius M; Beers, Timothy C; Moreno, Jorge Luis Meléndez; Ezzeddine, Rana; Casey, Andrew R; Hansen, Terese T; Roederer, Ian U; Sakari, Charli

    Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES

    Acesso à fonteDOIHow to cite
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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: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 28 jun. 2024.

    • 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 2024 jun. 28 ] 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 jun. 28 ] Available from: https://doi.org/10.3847/1538-4357/aad37d

  • Artigo de periodico

    G64-12 and G64-37 are carbon-enhanced metal-poor stars (2016)

    Placco, Vinicius M; Beers, Timothy C; Reggiani, Henrique; Moreno, Jorge Luis Meléndez

    Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR

    Acesso à fonteAcesso à fonteDOIHow to cite
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    • ABNT

      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: 28 jun. 2024.

    • APA

      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 jun. 28 ] 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 jun. 28 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
  • 1

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