Filtros : "MORENO, JORGE LUIS MELENDEZ" Removido: "2018" Limpar

Filtros



Refine with date range


  • Source: Astrophysical Journal Supplement Series. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 ago. 08 ] 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 ago. 08 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 ago. 08 ] 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 ago. 08 ] 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

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 ago. 08 ] 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 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stz3504
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROFISICA ESTELAR, SOL

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 ago. 08 ] 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 ago. 08 ] 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

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 2024 ago. 08 ] 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 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnrasl/slz153
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, PLANETAS

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 2024 ago. 08 ] 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 2024 ago. 08 ] 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

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      CARLOS, Marilia et al. The Li-age correlation: the sun is unusually Li deficient for its age. Monthly Notices of the Royal Astronomical Society, v. 485, p. 4052-4059, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 08 ago. 2024.
    • APA

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

      Carlos M, Moreno JLM, Spina L, dos Santos LA, Bedell M, Ramirez I, Asplund M, Bean JL, Yong D, Yana Galarza J, Alves-Brito A. The Li-age correlation: the sun is unusually Li deficient for its age [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 485 4052-4059.[citado 2024 ago. 08 ] 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 ago. 08 ] 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

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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 ago. 08 ] 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 ago. 08 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      SANTOS, Leonardo A. dos et al. Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions. Monthly Notices of the Royal Astronomical Society, v. 472, p. 3425-3436, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2199. Acesso em: 08 ago. 2024.
    • APA

      Santos, L. A. dos, Moreno, J. L. M., Bedell, M., Bean, J. L., Spina, L., Brito, A. A., et al. (2017). Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions. Monthly Notices of the Royal Astronomical Society, 472, 3425-3436. doi:10.1093/mnras/stx2199
    • NLM

      Santos LA dos, Moreno JLM, Bedell M, Bean JL, Spina L, Brito AA, Dreizler S, Ramírez I, Asplund M. Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 472 3425-3436.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stx2199
    • Vancouver

      Santos LA dos, Moreno JLM, Bedell M, Bean JL, Spina L, Brito AA, Dreizler S, Ramírez I, Asplund M. Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 472 3425-3436.[citado 2024 ago. 08 ] Available from: https://doi.org/10.1093/mnras/stx2199
  • Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.1093/mnras/stx047
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • 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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • 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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
  • Source: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Conference titles: IAU SYMPOSIUM. Unidade: IAG

    Subjects: ATIVIDADE SOLAR, ATIVIDADE ESTELAR, ESPECTROSCOPIA

    Acesso à fonteAcesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      MORENO, Jorge Luiz Meléndez e SANTOS, Leonardo A. dos e FREITAS, Fabrício C. Improved rotation-activity-age relations in Sun-like stars. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317004203. Acesso em: 08 ago. 2024.
    • APA

      Moreno, J. L. M., Santos, L. A. dos, & Freitas, F. C. (2017). Improved rotation-activity-age relations in Sun-like stars. In Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317004203
    • NLM

      Moreno JLM, Santos LA dos, Freitas FC. Improved rotation-activity-age relations in Sun-like stars [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 ago. 08 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317004203
    • Vancouver

      Moreno JLM, Santos LA dos, Freitas FC. Improved rotation-activity-age relations in Sun-like stars [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 ago. 08 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317004203
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • 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: 08 ago. 2024.
    • APA

      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. 08 ] 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. 08 ] Available from: https://doi.org/10.1051/0004-6361/201730560
  • Source: ASOS -12. Conference titles: International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

    How to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      TUCCI, M et al. The [Y/Mg] clock:: estimating stellar ages of solar-type stars. 2016, Anais.. São Paulo: IAG/USP, 2016. . Acesso em: 08 ago. 2024.
    • APA

      Tucci, M., Meléndez Moreno, J. L., Ramírez, I., Bedell, M., Bean, J., & Asplund, M. (2016). The [Y/Mg] clock:: estimating stellar ages of solar-type stars. In ASOS -12. São Paulo: IAG/USP.
    • NLM

      Tucci M, Meléndez Moreno JL, Ramírez I, Bedell M, Bean J, Asplund M. The [Y/Mg] clock:: estimating stellar ages of solar-type stars. ASOS -12. 2016 ;[citado 2024 ago. 08 ]
    • Vancouver

      Tucci M, Meléndez Moreno JL, Ramírez I, Bedell M, Bean J, Asplund M. The [Y/Mg] clock:: estimating stellar ages of solar-type stars. ASOS -12. 2016 ;[citado 2024 ago. 08 ]

Digital Library of Intellectual Production of Universidade de São Paulo     2012 - 2024