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  • Source: Astrophysical Journal Supplement Series. Unidade: IAG

    Subjects: 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://iopscience.iop.org/article/10.3847/1538-4365/ab9c19/pdf. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4365/ab9c19/pdf
    • 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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4365/ab9c19/pdf
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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      BOTELHO, R. B. et al. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc. Monthly Notices of the Royal Astronomical Society, v. 499, p. 2196-2213, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2917. Acesso em: 27 nov. 2022.
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      Botelho, R. B., Milone, A. de C., Moreno, J. L. M., Alves-Brito, A., Spina, L., & Bean, J. L. (2020). Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc. Monthly Notices of the Royal Astronomical Society, 499, 2196-2213. doi:10.1093/mnras/staa2917
    • NLM

      Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/staa2917
    • Vancouver

      Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: 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://iopscience.iop.org/article/10.3847/1538-4357/ab9c16/pdf. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9c16/pdf
    • 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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9c16/pdf
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: 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://iopscience.iop.org/article/10.3847/1538-4357/aad37d. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/aad37d
  • Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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      LORENZO-OLIVEIRA, Diego et al. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun. Monthly Notices of the Royal Astronomical Society Letters, v. 495, p. L61-L65, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2917. Acesso em: 27 nov. 2022.
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      Lorenzo-Oliveira, D., Moreno, J. L. M., Ponte, G., & Galarza, J. J. Y. (2020). The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun. Monthly Notices of the Royal Astronomical Society Letters, 495, L61-L65. doi:10.1093/mnrasl/slaa057
    • NLM

      Lorenzo-Oliveira D, Moreno JLM, Ponte G, Galarza JJY. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2020 ; 495 L61-L65.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/staa2917
    • Vancouver

      Lorenzo-Oliveira D, Moreno JLM, Ponte G, Galarza JJY. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2020 ; 495 L61-L65.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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      CARLOS, Marília et al. Li abundances for solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, v. 492, p. 245-249, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz3504. Acesso em: 27 nov. 2022.
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      Carlos, M., Milone, A. de C., Moreno, J. L. M., Nascimento Júnior, J. D. do, & Castro, M. (2020). Li abundances for solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 492, 245-249. doi:10.1093/mnras/stz3504
    • NLM

      Carlos M, Milone A de C, Moreno JLM, Nascimento Júnior JD do, Castro M. Li abundances for solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492 245-249.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/stz3504
    • Vancouver

      Carlos M, Milone A de C, Moreno JLM, Nascimento Júnior JD do, Castro M. Li abundances for solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492 245-249.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/stz3504
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: 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://iopscience.iop.org/article/10.3847/1538-4357/ab9d1a/pdf. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9d1a/pdf
    • 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 2022 nov. 27 ] Available from: https://iopscience.iop.org/article/10.3847/1538-4357/ab9d1a/pdf
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROFISICA ESTELAR, SOL

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      LORENZO-OLIVEIRA, Diego et al. Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 27 nov. 2022.
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      Lorenzo-Oliveira, D., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., Lambert, D. L., & Moreno, J. L. M. (2019). Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/slz034
    • NLM

      Lorenzo-Oliveira D, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL, Moreno JLM. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Lorenzo-Oliveira D, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL, Moreno JLM. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESPECTROMETRIA, ATMOSFERAS ESTELARES

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      GALARZA, Jhon Yana et al. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, v. 490, p. L86-L90, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slz153. Acesso em: 27 nov. 2022.
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      Galarza, J. Y., Meléndez, J., Lorenzo-Oliveira, D., Reggiani, H., Carlos, M., & Ponte, G. (2019). The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, 490, L86-L90. doi:10.1093/mnrasl/slz153
    • NLM

      Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnrasl/slz153
    • Vancouver

      Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnrasl/slz153
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, PLANETAS

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      BOTELHO, Roberto et al. Thorium in solar twins: implications for habitability in rocky planets. Monthly Notices of the Royal Astronomical Society, v. 482, p. 1690-1700, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 27 nov. 2022.
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      Botelho, R., Moreno, J. L. M., Alves-Brito, A., & Galarza, J. Y. (2019). Thorium in solar twins: implications for habitability in rocky planets. Monthly Notices of the Royal Astronomical Society, 482, 1690-1700. doi:10.1093/mnras/sty2791
    • NLM

      Botelho R, Moreno JLM, Alves-Brito A, Galarza JY. Thorium in solar twins: implications for habitability in rocky planets [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482 1690-1700.[citado 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Botelho R, Moreno JLM, Alves-Brito A, Galarza JY. Thorium in solar twins: implications for habitability in rocky planets [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482 1690-1700.[citado 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • 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: 27 nov. 2022.
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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
    • 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 2022 nov. 27 ] 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 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS BINARIAS

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      RAMIREZ, et al. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 27 nov. 2022.
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      Ramirez,, Khanal, S., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/sty104
    • NLM

      Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2022 nov. 27 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)

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      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: 27 nov. 2022.
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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 2022 nov. 27 ] 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 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/stx2938
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: 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, 2018Tradução . . Disponível em: http://doi.org/ 10.3847/1538-4357/ab8bd7. Acesso em: 27 nov. 2022.
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      Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2018). 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. 2018 ; 856( 2): 161-1/161-7.[citado 2022 nov. 27 ] Available from: http://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. 2018 ; 856( 2): 161-1/161-7.[citado 2022 nov. 27 ] Available from: http://doi.org/ 10.3847/1538-4357/ab8bd7
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: 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: 27 nov. 2022.
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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 2022 nov. 27 ] 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 2022 nov. 27 ] Available from: https://doi.org/10.1093/mnras/sty104
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: 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: http://doi.org/10.3847/1538-4357/aad190. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: http://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 2022 nov. 27 ] Available from: http://doi.org/10.3847/1538-4357/aad190
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: FORMAÇÃO DE ESTRELAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      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: 27 nov. 2022.
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      Liu, F., Ramírez, I., Lin, J., Yong, D., Asplund, M., Feltzing, S., 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, Ramírez I, Lin J, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM. 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 2022 nov. 27 ] Available from: https://doi.org/10.1051/0004-6361/201832701
    • Vancouver

      Liu F, Ramírez I, Lin J, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM. 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 2022 nov. 27 ] Available from: https://doi.org/10.1051/0004-6361/201832701
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

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    • ABNT

      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: http://doi.org/10.3847/1538-4357/aad908. Acesso em: 27 nov. 2022.
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      Bedell, M., Casagrande, L., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., 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, Casagrande L, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2022 nov. 27 ] Available from: http://doi.org/10.3847/1538-4357/aad908
    • Vancouver

      Bedell M, Casagrande L, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2022 nov. 27 ] Available from: http://doi.org/10.3847/1538-4357/aad908
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: 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: http://doi.org/10.3847/1538-4357/aab36c. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: http://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 2022 nov. 27 ] Available from: http://doi.org/10.3847/1538-4357/aab36c
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES

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    • ABNT

      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: http://doi.org/10.3847/1538-4357/aad37d. Acesso em: 27 nov. 2022.
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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 2022 nov. 27 ] Available from: http://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 2022 nov. 27 ] Available from: http://doi.org/10.3847/1538-4357/aad37d

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