Filtros : "MORENO, JORGE LUIS MELENDEZ" "ABUNDÂNCIA ESTELAR" Removido: "2019" Limpar

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  • Fonte: Astrophysical Journal Supplement Series. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      HOLMBECK, Erika M. The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo*. Astrophysical Journal Supplement Series, v. 249, p. 30, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/ab9c19. Acesso em: 09 ago. 2024.
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      Holmbeck, E. M. (2020). The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo*. Astrophysical Journal Supplement Series, 249, 30. doi:10.3847/1538-4365/ab9c19
    • NLM

      Holmbeck EM. The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo* [Internet]. Astrophysical Journal Supplement Series. 2020 ; 249 30.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
    • Vancouver

      Holmbeck EM. The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo* [Internet]. Astrophysical Journal Supplement Series. 2020 ; 249 30.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e GALARZA, Jhon J. Yana. How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab8bd7. Acesso em: 09 ago. 2024.
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      Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2020). How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/ab8bd7
    • NLM

      Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
    • Vancouver

      Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      NASCIMENTO J.-D. DO, et al. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, v. 898, p. 173 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab9c16. Acesso em: 09 ago. 2024.
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      Nascimento J.-D. do,, Almeida, L. de, Velloso, E. N., Anthony, F., Costa, J. S. da, Castro, M., & Moreno, J. L. M. (2020). Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, 898, 173 2020. doi:10.3847/1538-4357/ab9c16
    • NLM

      Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
    • Vancouver

      Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      CAIN, Madelyn e MORENO, Jorge Luis Meléndez. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, v. 864, p. 43 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 09 ago. 2024.
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      Cain, M., & Moreno, J. L. M. (2020). The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, 864, 43 2020. doi:10.3847/1538-4357/aad37d
    • NLM

      Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
    • Vancouver

      Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      EZZEDDINE, Rana e MORENO, Jorge Luis Meléndez. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, v. 898, p. 150 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d1a. Acesso em: 09 ago. 2024.
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      Ezzeddine, R., & Moreno, J. L. M. (2020). The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, 898, 150 2020. doi:10.3847/1538-4357/aad37d1a
    • NLM

      Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
    • Vancouver

      Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)

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    • ABNT

      SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e ALVES-BRITO, Alan. The temporal evolution of neutron-capture elements in the Galactic discs. Monthly Notices of the Royal Astronomical Society, v. 474, n. 2, p. 2580-2593, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2938. Acesso em: 09 ago. 2024.
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      Spina, L., Moreno, J. L. M., & Alves-Brito, A. (2018). The temporal evolution of neutron-capture elements in the Galactic discs. Monthly Notices of the Royal Astronomical Society, 474( 2), 2580-2593. doi:10.1093/mnras/stx2938
    • NLM

      Spina L, Moreno JLM, Alves-Brito A. The temporal evolution of neutron-capture elements in the Galactic discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 474( 2): 2580-2593.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1093/mnras/stx2938
    • Vancouver

      Spina L, Moreno JLM, Alves-Brito A. The temporal evolution of neutron-capture elements in the Galactic discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 474( 2): 2580-2593.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1093/mnras/stx2938
  • Fonte: Astronomy & Astrophysics. Unidade: IAG

    Assuntos: 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: 09 ago. 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 ago. 09 ] 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 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201832701
  • Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      REGGIANI, Henrique e MORENO, Jorge Luis Meléndez. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440. Monthly Notices of the Royal Astronomical Society, v. 475, n. 3, p. 3502-3510, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty104. Acesso em: 09 ago. 2024.
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      Reggiani, H., & Moreno, J. L. M. (2018). Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440. Monthly Notices of the Royal Astronomical Society, 475( 3), 3502-3510. doi:10.1093/mnras/sty104
    • NLM

      Reggiani H, Moreno JLM. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 3502-3510.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1093/mnras/sty104
    • Vancouver

      Reggiani H, Moreno JLM. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 3502-3510.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1093/mnras/sty104
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      SPINA, Lorenzo et al. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, v. 863, n. 2, p. 179-1/179-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 09 ago. 2024.
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      Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
    • NLM

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad190
    • Vancouver

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad190
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

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      BEDELL, Megan et al. The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, v. 865, n. 1, p. 68-1/68-13, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad908. Acesso em: 09 ago. 2024.
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      Bedell, M., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., Asplund, M., et al. (2018). The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, 865( 1), 68-1/68-13. doi:10.3847/1538-4357/aad908
    • NLM

      Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad908
    • Vancouver

      Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad908
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      CARLOS, Marília et al. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 09 ago. 2024.
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      Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
    • NLM

      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
    • Vancouver

      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
  • Fonte: Astronomy and Astrophysysics. Unidade: IAG

    Assuntos: PLANETAS, ABUNDÂNCIA ESTELAR

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      LORENZO-OLIVEIRA, Diego et al. The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, v. 619, p. A73, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629294. Acesso em: 09 ago. 2024.
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      Lorenzo-Oliveira, D., Freitas, F. C., Moreno, J. L. M., & Bedell, M. (2018). The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, 619, A73. doi:10.1051/0004-6361/201629294
    • NLM

      Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201629294
    • Vancouver

      Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201629294
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES

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      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: 09 ago. 2024.
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      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 ago. 09 ] 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 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Fonte: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Assuntos: 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: 09 ago. 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 ago. 09 ] 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 ago. 09 ] Available from: https://doi.org/10.1093/mnras/stx047
  • Fonte: Astronomy and Astrophysysics. Unidade: IAG

    Assuntos: PLANETAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      MORENO, Jorge Luiz Meléndez et al. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, v. 597, p. A34, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527775. Acesso em: 09 ago. 2024.
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      Moreno, J. L. M., Bedell, M., Bean, J. L., Mello, S. F., Galarza, J. Y., Santos, L. dos, et al. (2017). The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, 597, A34. doi:10.1051/0004-6361/201527775
    • NLM

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201527775
    • Vancouver

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • Fonte: Astrophysical Journal. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, PLANETAS

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    • ABNT

      BEDELL, Megan et al. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, v. 839, p. 94. 2017, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6a1d. Acesso em: 09 ago. 2024.
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      Bedell, M., Bean, J. L., Moreno, J. L. M., Mills, S. M., Fabrycky, D. C., Freitas, F. C., et al. (2017). Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, 839, 94. 2017. doi:10.3847/1538-4357/aa6a1d
    • NLM

      Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
    • Vancouver

      Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 ago. 09 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
  • Fonte: Astronomy & Astrophysics. Unidade: IAG

    Assuntos: GALÁXIAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      BENSBY, T e MORENO, Jorge Luis Meléndez. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, v. 605, p. 89, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730560. Acesso em: 09 ago. 2024.
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      Bensby, T., & Moreno, J. L. M. (2017). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, 605, 89. doi:10.1051/0004-6361/201730560
    • NLM

      Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201730560
    • Vancouver

      Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201730560
  • Fonte: Astronomy & Astrophysics. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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    • ABNT

      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: 09 ago. 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
    • 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 ; 590 A66/1-A66/8.[citado 2024 ago. 09 ] 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 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201526643
  • Fonte: Astronomy & Astrophysics. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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    • ABNT

      SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 09 ago. 2024.
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      Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
    • NLM

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201527429
    • Vancouver

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201527429
  • Fonte: Astronomy & Astrophysics. Unidade: IAG

    Assuntos: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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    • ABNT

      REGGIANI, Henrique et al. First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, v. 586, p. A67/1-A67/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527439. Acesso em: 09 ago. 2024.
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      Reggiani, H., Moreno, J. L. M., Yong, D., Ramírez, I., & Asplund, M. (2016). First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, 586, A67/1-A67/8. doi:10.1051/0004-6361/201527439
    • NLM

      Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201527439
    • Vancouver

      Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 ago. 09 ] Available from: https://doi.org/10.1051/0004-6361/201527439

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