Filtros : "Yong, D" Limpar

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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: SOL, ABUNDÂNCIAS SOLARES, ESTRELAS, ABUNDÂNCIA ESTELAR, TERRA (PLANETA), METEOROS

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      MELÉNDEZ MORENO, Jorge Luis et al. The remarkable solar twin HIP 56948: a prime target in the quest for other Earths. Astronomy & Astrophysics, v. 543, p. A29/1-A29/27, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201117222. Acesso em: 18 abr. 2024.
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      Meléndez Moreno, J. L., Bergmann, M., Cohen, J. G., Endl, M., Karakas, A. I., Ramírez, I., et al. (2012). The remarkable solar twin HIP 56948: a prime target in the quest for other Earths. Astronomy & Astrophysics, 543, A29/1-A29/27. doi:10.1051/0004-6361/201117222
    • NLM

      Meléndez Moreno JL, Bergmann M, Cohen JG, Endl M, Karakas AI, Ramírez I, Cochran WD, Yong D, MacQueen PJ, Kobayashi C, Asplund M. The remarkable solar twin HIP 56948: a prime target in the quest for other Earths [Internet]. Astronomy & Astrophysics. 2012 ; 543 A29/1-A29/27.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201117222
    • Vancouver

      Meléndez Moreno JL, Bergmann M, Cohen JG, Endl M, Karakas AI, Ramírez I, Cochran WD, Yong D, MacQueen PJ, Kobayashi C, Asplund M. The remarkable solar twin HIP 56948: a prime target in the quest for other Earths [Internet]. Astronomy & Astrophysics. 2012 ; 543 A29/1-A29/27.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201117222
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS

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      RAMÍREZ, I et al. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, v. 808, p. 13/1-13/14, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/13. Acesso em: 18 abr. 2024.
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      Ramírez, I., Khanal, S., Aleo, P., Sobotka, A., Liu, F., Casagrande, L., et al. (2015). The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, 808, 13/1-13/14. doi:10.1088/0004-637X/808/1/13
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      Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
    • Vancouver

      Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
  • 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: 18 abr. 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 abr. 18 ] 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 abr. 18 ] Available from: https://doi.org/10.1093/mnras/stv2821
  • 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: 18 abr. 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
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      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 abr. 18 ] Available from: https://doi.org/10.1093/mnras/stw2045
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      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 abr. 18 ] 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: 18 abr. 2024.
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      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 abr. 18 ] 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 abr. 18 ] Available from: https://doi.org/10.1093/mnras/stw2045
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 590, p. A66/1-A66/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526643. Acesso em: 18 abr. 2024.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 590, A66/1-A66/8. doi:10.1051/0004-6361/201526643
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      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 590 A66/1-A66/8.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201526643
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 590 A66/1-A66/8.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201526643
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 18 abr. 2024.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 588, A66. doi:10.1051/0004-6361/201526643
    • NLM

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 abr. 18 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 abr. 18 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns. Astronomy & Astrophysics, v. 572, p. A108/1-A108/21, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424533. Acesso em: 18 abr. 2024.
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      Thygesen, A. O., Sbordone, L., Andrievsky, S., Korotin, S., Yong, D., Zaggia, S., et al. (2014). The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns. Astronomy & Astrophysics, 572, A108/1-A108/21. doi:10.1051/0004-6361/201424533
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      Thygesen AO, Sbordone L, Andrievsky S, Korotin S, Yong D, Zaggia S, Ludwig H-G, Collet R, Asplund M, Ventura P, D'Antona F, Moreno JLM, D'Ercole A. The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns [Internet]. Astronomy & Astrophysics. 2014 ; 572 A108/1-A108/21.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201424533
    • Vancouver

      Thygesen AO, Sbordone L, Andrievsky S, Korotin S, Yong D, Zaggia S, Ludwig H-G, Collet R, Asplund M, Ventura P, D'Antona F, Moreno JLM, D'Ercole A. The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns [Internet]. Astronomy & Astrophysics. 2014 ; 572 A108/1-A108/21.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201424533
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ABUNDANCIAS SOLARES

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      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: 18 abr. 2024.
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      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
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      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 abr. 18 ] 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 abr. 18 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • 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: 18 abr. 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
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      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 abr. 18 ] 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 abr. 18 ] Available from: https://doi.org/10.1093/mnras/stw247
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: SOL, ABUNDÂNCIAS SOLARES, ATMOSFERA, ABUNDÂNCIA ESTELAR, ESTRELAS

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      TUCCI MAIA, M et al. Shallow extra mixing in solar twins inferred from Be abundances. Astronomy & Astrophysics, v. 576, p. L10/1-L10/4, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201425357. Acesso em: 18 abr. 2024.
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      Tucci Maia, M., Moreno, J. L. M., Castro, M., Asplund, M., Ramírez, I., Monroe, T. R., et al. (2015). Shallow extra mixing in solar twins inferred from Be abundances. Astronomy & Astrophysics, 576, L10/1-L10/4. doi:10.1051/0004-6361/201425357
    • NLM

      Tucci Maia M, Moreno JLM, Castro M, Asplund M, Ramírez I, Monroe TR, Nascimento Jr. J-D do, Yong D. Shallow extra mixing in solar twins inferred from Be abundances [Internet]. Astronomy & Astrophysics. 2015 ; 576 L10/1-L10/4.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201425357
    • Vancouver

      Tucci Maia M, Moreno JLM, Castro M, Asplund M, Ramírez I, Monroe TR, Nascimento Jr. J-D do, Yong D. Shallow extra mixing in solar twins inferred from Be abundances [Internet]. Astronomy & Astrophysics. 2015 ; 576 L10/1-L10/4.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201425357
  • Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      FISHLOCK, C. K et al. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 466, p. 4672-4682, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx047. Acesso em: 18 abr. 2024.
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      Fishlock, C. K., Yong, D., Karakas, A. I., Alves-Brito, A., Moreno, J. L. M., Nissen, P. E., et al. (2017). Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 466, 4672-4682. doi:10.1093/mnras/stx047
    • NLM

      Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1093/mnras/stx047
    • Vancouver

      Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1093/mnras/stx047
  • 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: 18 abr. 2024.
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      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
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      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 abr. 18 ] 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 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201628557
  • 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: 18 abr. 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
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      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 abr. 18 ] 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 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201832701
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), ABUNDÂNCIA ESTELAR

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      ALVES-BRITO, A et al. CNO and F abundances in the globular cluster M22 (NGC 6656). Astronomy & Astrophysics, v. 540, p. A3/1-A3/12, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118623. Acesso em: 18 abr. 2024.
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      Alves-Brito, A., Yong, D., Meléndez Moreno, J. L., Vásquez, S., & Karakas, A. I. (2012). CNO and F abundances in the globular cluster M22 (NGC 6656). Astronomy & Astrophysics, 540, A3/1-A3/12. doi:10.1051/0004-6361/201118623
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      Alves-Brito A, Yong D, Meléndez Moreno JL, Vásquez S, Karakas AI. CNO and F abundances in the globular cluster M22 (NGC 6656) [Internet]. Astronomy & Astrophysics. 2012 ; 540 A3/1-A3/12.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201118623
    • Vancouver

      Alves-Brito A, Yong D, Meléndez Moreno JL, Vásquez S, Karakas AI. CNO and F abundances in the globular cluster M22 (NGC 6656) [Internet]. Astronomy & Astrophysics. 2012 ; 540 A3/1-A3/12.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1051/0004-6361/201118623
  • Source: ASP Conference Series. Conference titles: Subaru International Conference. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA)

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      BENSBY, T et al. Abundance trends in the inner and outer galactic disk. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 18 abr. 2024. , 2012
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      Bensby, T., Alves-Brito, A., Oey, M. S., Yong, D., & Moreno, J. L. M. (2012). Abundance trends in the inner and outer galactic disk. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
    • NLM

      Bensby T, Alves-Brito A, Oey MS, Yong D, Moreno JLM. Abundance trends in the inner and outer galactic disk. ASP Conference Series. 2012 ; 458 171-174.[citado 2024 abr. 18 ]
    • Vancouver

      Bensby T, Alves-Brito A, Oey MS, Yong D, Moreno JLM. Abundance trends in the inner and outer galactic disk. ASP Conference Series. 2012 ; 458 171-174.[citado 2024 abr. 18 ]
  • Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, FORMAÇÃO DO SISTEMA SOLAR, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS BINÁRIAS

    Acesso à fonteDOIHow to cite
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    • ABNT

      LIU, F et al. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, v. 442, p. L51-L55, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slu055. Acesso em: 18 abr. 2024.
    • APA

      Liu, F., Asplund, M., Ramírez, I., Yong, D., & Moreno, J. L. M. (2014). A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, 442, L51-L55. doi:10.1093/mnrasl/slu055
    • NLM

      Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1093/mnrasl/slu055
    • Vancouver

      Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 abr. 18 ] Available from: https://doi.org/10.1093/mnrasl/slu055

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