Filtros : "ABUNDÂNCIA ESTELAR" "Reino Unido" "The Astrophysical Journal Letters" Limpar

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  • 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: 16 out. 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 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: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS, SOL

    Acesso à fonteDOIHow to cite
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    • ABNT

      NASCIMENTO JÚNIOR, J.-D. do et al. The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, v. 771, p. L31/1-L31/5, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/771/2/L31. Acesso em: 16 out. 2024.
    • APA

      Nascimento Júnior, J. -D. do, Takeda, Y., Moreno, J. L. M., Costa, J. S. da, Mello, G. F. P. de, & Castro, M. (2013). The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, 771, L31/1-L31/5. doi:10.1088/2041-8205/771/2/L31
    • NLM

      Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 out. 16 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
    • Vancouver

      Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 out. 16 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

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    • ABNT

      MONROE, Tala Wanda R et al. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun. The Astrophysical Journal Letters, v. 774, p. L32/1-L32/6, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/774/2/L32. Acesso em: 16 out. 2024.
    • APA

      Monroe, T. W. R., Moreno, J. L. M., Maia, M. T., & Freitas, F. C. (2013). High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun. The Astrophysical Journal Letters, 774, L32/1-L32/6. doi:10.1088/2041-8205/774/2/L32
    • NLM

      Monroe TWR, Moreno JLM, Maia MT, Freitas FC. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun [Internet]. The Astrophysical Journal Letters. 2013 ; 774 L32/1-L32/6.[citado 2024 out. 16 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
    • Vancouver

      Monroe TWR, Moreno JLM, Maia MT, Freitas FC. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun [Internet]. The Astrophysical Journal Letters. 2013 ; 774 L32/1-L32/6.[citado 2024 out. 16 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, ABUNDÂNCIA ESTELAR

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    • ABNT

      BENSBY, T et al. A first constraint on the thick disk scale length: differential radial abundances in K giants at galactocentric radii 4, 8, and 12 kpc. The Astrophysical Journal Letters, v. 735, p. L46/1-L46/6, 2011Tradução . . Acesso em: 16 out. 2024.
    • APA

      Bensby, T., Alves-Brito, A., Oey, M. S., Yong, D., & Moreno, J. L. M. (2011). A first constraint on the thick disk scale length: differential radial abundances in K giants at galactocentric radii 4, 8, and 12 kpc. The Astrophysical Journal Letters, 735, L46/1-L46/6.
    • NLM

      Bensby T, Alves-Brito A, Oey MS, Yong D, Moreno JLM. A first constraint on the thick disk scale length: differential radial abundances in K giants at galactocentric radii 4, 8, and 12 kpc. The Astrophysical Journal Letters. 2011 ; 735 L46/1-L46/6.[citado 2024 out. 16 ]
    • Vancouver

      Bensby T, Alves-Brito A, Oey MS, Yong D, Moreno JLM. A first constraint on the thick disk scale length: differential radial abundances in K giants at galactocentric radii 4, 8, and 12 kpc. The Astrophysical Journal Letters. 2011 ; 735 L46/1-L46/6.[citado 2024 out. 16 ]

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