Filtros : "IAG" "ABUNDÂNCIA ESTELAR" "Australian National University, Weston Creek, Australia" Removidos: "Índia" "LIMA, JOSÉ ADEMIR SALES DE" Limpar

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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, CINEMÁTICA, DINÂMICA, POPULAÇÕES ESTELARES, GALÁXIA (VIA LÁCTEA)

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, v. 573, p. A13/1-A13/23, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423996. Acesso em: 05 jun. 2024.
    • APA

      Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Costa, G. S. da, Ortolani, S., et al. (2015). FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, 573, A13/1-A13/23. doi:10.1051/0004-6361/201423996
    • NLM

      Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201423996
    • Vancouver

      Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201423996
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESPECTROSCOPIA

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      LIND, K et al. The lithium isotopic ratio in very metal-poor stars. Astronomy & Astrophysics, v. 554, p. A96/1-A96/15, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201321406. Acesso em: 05 jun. 2024.
    • APA

      Lind, K., Moreno, J. L. M., Asplund, M., Collet, R., & Magic, Z. (2013). The lithium isotopic ratio in very metal-poor stars. Astronomy & Astrophysics, 554, A96/1-A96/15. doi:10.1051/0004-6361/201321406
    • NLM

      Lind K, Moreno JLM, Asplund M, Collet R, Magic Z. The lithium isotopic ratio in very metal-poor stars [Internet]. Astronomy & Astrophysics. 2013 ; 554 A96/1-A96/15.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201321406
    • Vancouver

      Lind K, Moreno JLM, Asplund M, Collet R, Magic Z. The lithium isotopic ratio in very metal-poor stars [Internet]. Astronomy & Astrophysics. 2013 ; 554 A96/1-A96/15.[citado 2024 jun. 05 ] Available from: https://doi.org/10.1051/0004-6361/201321406

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