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Filtros : "MORENO, JORGE LUIS MELENDEZ" Removido: "Galarza, Jhon Yana" Limpar

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  • Artigo de periodico

    The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo* (2020)

    Holmbeck, Erika M.

    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://doi.org/10.3847/1538-4365/ab9c19. Acesso em: 15 out. 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

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      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19

  • Artigo de periodico

    How Magnetic Activity Alters What We Learn from Stellar Spectra (2020)

    Spina, Lorenzo ; Moreno, Jorge Luis Meléndez ; Galarza, Jhon J. Yana

    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, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab8bd7. Acesso em: 15 out. 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

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      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7

  • Artigo de periodico

    Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc (2020)

    Botelho, R. B. ; Milone, A de C. ; Moreno, Jorge Luiz Meléndez ; Alves-Brito, A. ; Spina, L ; Bean, J L

    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: 15 out. 2024.

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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 2024 out. 15 ] 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 2024 out. 15 ] Available from: https://doi.org/10.1093/mnras/staa2917

  • Artigo de periodico

    Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 (2020)

    Nascimento J.-D. do ; Almeida, L. de ; Velloso, E. N ; Anthony, F.; Costa, J. S. da; Castro, M; Moreno, Jorge Luis Meléndez

    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://doi.org/10.3847/1538-4357/ab9c16. Acesso em: 15 out. 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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16

  • Artigo de periodico

    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 (2020)

    Cain,Madelyn ; Moreno, Jorge Luis Meléndez

    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://doi.org/10.3847/1538-4357/aad37d. Acesso em: 15 out. 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

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      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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad37d

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      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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad37d

  • Artigo de periodico

    The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun (2020)

    Lorenzo-Oliveira, Diego ; Moreno, Jorge Luis Meléndez ; Ponte, Geisa ; Galarza, Jhon J. Yana

    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: 15 out. 2024.

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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/mnras/staa2917

    • 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 2024 out. 15 ] 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 2024 out. 15 ] Available from: https://doi.org/10.1093/mnras/staa2917

  • Artigo de periodico

    Li abundances for solar twins in the open cluster M67 (2020)

    Carlos, Marília; Milone, A de C. ; Moreno, Jorge Luiz Meléndez ; Nascimento Júnior, José Dias do; Castro, Matthieu

    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: 15 out. 2024.

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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 2024 out. 15 ] 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 2024 out. 15 ] Available from: https://doi.org/10.1093/mnras/stz3504

  • Artigo de periodico

    The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* (2020)

    Ezzeddine, Rana; Moreno, Jorge Luis Meléndez

    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://doi.org/10.3847/1538-4357/aad37d1a. Acesso em: 15 out. 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

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      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a

  • Artigo de periodico

    Constraining teh evolutionofstellar rotation using solar twins (2019)

    Lorenzo-Oliveira, Diego; Moreno, Jorge Luiz Meléndez; Lichon, S. J; Chanamé, J; Endl, M; Moreno, Jorge Luis Meléndez; Lambert, D. L.

    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: 15 out. 2024.

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      Lorenzo-Oliveira, D., Moreno, J. L. M., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (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, Moreno JLM, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 out. 15 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050

    • Vancouver

      Lorenzo-Oliveira D, Moreno JLM, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 out. 15 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050

  • Artigo de periodico

    The Li-age correlation: the sun is unusually Li deficient for its age (2019)

    Carlos, Marilia; Moreno, Jorge Luiz Meléndez ; Spina, L; dos Santos, L. A; Bedell, M; Ramirez, I; Asplund, M; Bean, J. L; Yong, D; Yana Galarza, J; Alves-Brito, A

    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: 15 out. 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

    • 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 out. 15 ] 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 out. 15 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050

  • Artigo de periodico

    The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs (2019)

    Ramirez; Khanal, S.; Lichon, S. J; Chanamé, J; Endl, M; Moreno, Jorge Luis Meléndez; Lambert, D. L.

    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: 15 out. 2024.

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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 2024 out. 15 ] 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 2024 out. 15 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050

  • Artigo de periodico

    The temporal evolution of neutron-capture elements in the Galactic discs (2018)

    Spina, Lorenzo; Moreno, Jorge Luis Meléndez; Alves-Brito, Alan

    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: 15 out. 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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1093/mnras/stx2938

  • Artigo de periodico

    Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation (2018)

    Liu, F; Yong, D; Asplund, M; Feltzing, S; Mustill, A. J; Moreno, Jorge Luis Meléndez; Ramírez, I; Lin, J

    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: 15 out. 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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201832701

  • Artigo de periodico

    Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 (2018)

    Reggiani, Henrique; Moreno, Jorge Luis Meléndez

    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: 15 out. 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

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      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1093/mnras/sty104

  • Artigo de periodico

    Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres (2018)

    Spina, Lorenzo; Moreno, Jorge Luis Meléndez; Casey, Andrew R; Karakas, Amanda I; Tucci-Maia, Marcelo

    Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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    • ABNT

      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: 15 out. 2024.

    • APA

      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad190

  • Artigo de periodico

    The chemical homogeneity of sun-like stars in the solar neighborhood (2018)

    Bedell, Megan; Bean, Jacob L; Moreno, Jorge Luis Meléndez; Spina, Lorenzo; Ramirez, Ivan; Asplund, Martin; Alves-Brito, Alan; Santos, Leonardo dos; Dreizler, Stefan; Yong, David; Monroe, TalaWanda; Casagrande, Luca

    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: https://doi.org/10.3847/1538-4357/aad908. Acesso em: 15 out. 2024.

    • APA

      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad908

  • Artigo de periodico

    A formation timescale of the galactic Halo from Mg isotopes in dwarf stars (2018)

    Carlos, Marília; Karakas, Amanda I; Cohen, Judith G; Kobayashi, Chiaki; Moreno, Jorge Luis Meléndez

    Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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    • ABNT

      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: 15 out. 2024.

    • APA

      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aab36c

  • Artigo de periodico

    The solar twin planet search: The age - chromospheric activity relation (2018)

    Lorenzo-Oliveira, Diego; Freitas, Fabrício C; Moreno, Jorge Luiz Meléndez; Bedell, Megan

    Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      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: 15 out. 2024.

    • APA

      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201629294

  • Artigo de periodico

    Modelling the solar twin 18 Scorpii (2018)

    Bazot, M; Creevey, O; Christensen-Dalsgaard, J; Moreno, Jorge Luis Meléndez

    Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, EVOLUÇÃO ESTELAR

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    • ABNT

      BAZOT, M et al. Modelling the solar twin 18 Scorpii. Astronomy & Astrophysics, v. 619, p. A172, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834058. Acesso em: 15 out. 2024.

    • APA

      Bazot, M., Creevey, O., Christensen-Dalsgaard, J., & Moreno, J. L. M. (2018). Modelling the solar twin 18 Scorpii. Astronomy & Astrophysics, 619, A172. doi:10.1051/0004-6361/201834058

    • NLM

      Bazot M, Creevey O, Christensen-Dalsgaard J, Moreno JLM. Modelling the solar twin 18 Scorpii [Internet]. Astronomy & Astrophysics. 2018 ; 619 A172.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201834058

    • Vancouver

      Bazot M, Creevey O, Christensen-Dalsgaard J, Moreno JLM. Modelling the solar twin 18 Scorpii [Internet]. Astronomy & Astrophysics. 2018 ; 619 A172.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201834058

  • Artigo de periodico

    The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild (2018)

    Cain, Madelyn; Frebel, Anna; Gull, Maude; Ji, Alexander P; Placco, Vinicius M; Beers, Timothy C; Moreno, Jorge Luis Meléndez; Ezzeddine, Rana; Casey, Andrew R; Hansen, Terese T; Roederer, Ian U; Sakari, Charli

    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: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 15 out. 2024.

    • APA

      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad37d

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