Filtros : "Austrália" "Asplund, M" Removidos: "SHIMA, HISAKO" "Rezende, Magda Andrade" "Indexado no: CUIDEN" "Teixeira, Manoel Jacobsen" Limpar

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  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ABUNDANCIAS SOLARES

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    • ABNT

      CARLOS, Marilia et al. The Li-age correlation: the sun is unusually Li deficient for its age. Monthly Notices of the Royal Astronomical Society, v. 485, p. 4052-4059, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 31 maio 2024.
    • APA

      Carlos, M., Moreno, J. L. M., Spina, L., dos Santos, L. A., Bedell, M., Ramirez, I., et al. (2019). The Li-age correlation: the sun is unusually Li deficient for its age. Monthly Notices of the Royal Astronomical Society, 485, 4052-4059. doi:10.1093/mnras/slz681
    • NLM

      Carlos M, Moreno JLM, Spina L, dos Santos LA, Bedell M, Ramirez I, Asplund M, Bean JL, Yong D, Yana Galarza J, Alves-Brito A. The Li-age correlation: the sun is unusually Li deficient for its age [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 485 4052-4059.[citado 2024 maio 31 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Carlos M, Moreno JLM, Spina L, dos Santos LA, Bedell M, Ramirez I, Asplund M, Bean JL, Yong D, Yana Galarza J, Alves-Brito A. The Li-age correlation: the sun is unusually Li deficient for its age [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 485 4052-4059.[citado 2024 maio 31 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: FORMAÇÃO DE ESTRELAS, ABUNDÂNCIA ESTELAR

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      LIU, F et al. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation. Astronomy & Astrophysics, v. 614, p. A138, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201832701. Acesso em: 31 maio 2024.
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      Liu, F., Yong, D., Asplund, M., Feltzing, S., Mustill, A. J., Moreno, J. L. M., et al. (2018). Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation. Astronomy & Astrophysics, 614, A138. doi:10.1051/0004-6361/201832701
    • NLM

      Liu F, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM, Ramírez I, Lin J. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation [Internet]. Astronomy & Astrophysics. 2018 ; 614 A138.[citado 2024 maio 31 ] Available from: https://doi.org/10.1051/0004-6361/201832701
    • Vancouver

      Liu F, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM, Ramírez I, Lin J. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation [Internet]. Astronomy & Astrophysics. 2018 ; 614 A138.[citado 2024 maio 31 ] Available from: https://doi.org/10.1051/0004-6361/201832701
  • 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: 31 maio 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 maio 31 ] 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 maio 31 ] Available from: https://doi.org/10.1093/mnras/stw247
  • 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: 31 maio 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 maio 31 ] 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 maio 31 ] Available from: https://doi.org/10.1093/mnras/stv2821
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS

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      SPINA, L. et al. Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy. Astronomy & Astrophysics, v. 59, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628557. Acesso em: 31 maio 2024.
    • APA

      Spina, L., Moreno, J. L. M., Karakas, A. I., Ramírez, I., Monroe, T. R., Asplund, M., & Yong, D. (2016). Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy. Astronomy & Astrophysics, 59. doi:10.1051/0004-6361/201628557
    • NLM

      Spina L, Moreno JLM, Karakas AI, Ramírez I, Monroe TR, Asplund M, Yong D. Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy [Internet]. Astronomy & Astrophysics. 2016 ; 59[citado 2024 maio 31 ] Available from: https://doi.org/10.1051/0004-6361/201628557
    • Vancouver

      Spina L, Moreno JLM, Karakas AI, Ramírez I, Monroe TR, Asplund M, Yong D. Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy [Internet]. Astronomy & Astrophysics. 2016 ; 59[citado 2024 maio 31 ] Available from: https://doi.org/10.1051/0004-6361/201628557
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      TUCCI MAIA, M et al. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars. Astronomy & Astrophysics, v. 590, p. A32/1-A32/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527848. Acesso em: 31 maio 2024.
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      Tucci Maia, M., Ramírez, I., Moreno, J. L. M., Bedell, M., Bean, J. L., & Asplund, M. (2016). The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars. Astronomy & Astrophysics, 590, A32/1-A32/8. doi:10.1051/0004-6361/201527848
    • NLM

      Tucci Maia M, Ramírez I, Moreno JLM, Bedell M, Bean JL, Asplund M. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars [Internet]. Astronomy & Astrophysics. 2016 ; 590 A32/1-A32/8.[citado 2024 maio 31 ] Available from: https://doi.org/10.1051/0004-6361/201527848
    • Vancouver

      Tucci Maia M, Ramírez I, Moreno JLM, Bedell M, Bean JL, Asplund M. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars [Internet]. Astronomy & Astrophysics. 2016 ; 590 A32/1-A32/8.[citado 2024 maio 31 ] Available from: https://doi.org/10.1051/0004-6361/201527848
  • 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: 31 maio 2024.
    • APA

      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 maio 31 ] 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 maio 31 ] Available from: https://doi.org/10.1093/mnras/stw2045

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