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  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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    • 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: 07 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
    • 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 out. 07 ] 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. 07 ] 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

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    • 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: 07 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. 07 ] 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. 07 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • Source: Royal Astronomical Society. Monthly Notices. Unidades: IAG, EACH

    Subjects: FORMAÇÃO DE ESTRELAS, MEIO INTERESTELAR

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      AKHTER, Shaila et al. Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS. Royal Astronomical Society. Monthly Notices, p. 01-29, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa267. Acesso em: 07 out. 2024.
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      Akhter, S., Cunningham, M. R., Harvey-Smith, L., Nawaz, M. A., Jones, P. A., Walsh, A., et al. (2020). Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS. Royal Astronomical Society. Monthly Notices, 01-29. doi:10.1093/mnras/staa267
    • NLM

      Akhter S, Cunningham MR, Harvey-Smith L, Nawaz MA, Jones PA, Walsh A, Dal Pino EM de G, Falceta Gonçalves DA. Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS [Internet]. Royal Astronomical Society. Monthly Notices. 2020 ; 01-29.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/staa267
    • Vancouver

      Akhter S, Cunningham MR, Harvey-Smith L, Nawaz MA, Jones PA, Walsh A, Dal Pino EM de G, Falceta Gonçalves DA. Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS [Internet]. Royal Astronomical Society. Monthly Notices. 2020 ; 01-29.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/staa267
  • 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: 07 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. 07 ] 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. 07 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: ASTROMETRIA

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    • ABNT

      DIAS, W.S et al. Astrometric and photometric study of Dias 4, Dias 6, and other five open clusters using ground-based and Gaia DR2 data. Monthly Notices of the Royal Astronomical Society, v. 481, n. 3, p. 3887-3901, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty2341. Acesso em: 07 out. 2024.
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      Dias, W. S., Monteiro, H., Lépine, J. R. D., Prates, R., Gneiding, C. D., & Sacchi, M. (2018). Astrometric and photometric study of Dias 4, Dias 6, and other five open clusters using ground-based and Gaia DR2 data. Monthly Notices of the Royal Astronomical Society, 481( 3), 3887-3901. doi:10.1093/mnras/sty2341
    • NLM

      Dias WS, Monteiro H, Lépine JRD, Prates R, Gneiding CD, Sacchi M. Astrometric and photometric study of Dias 4, Dias 6, and other five open clusters using ground-based and Gaia DR2 data [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 481( 3): 3887-3901.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/sty2341
    • Vancouver

      Dias WS, Monteiro H, Lépine JRD, Prates R, Gneiding CD, Sacchi M. Astrometric and photometric study of Dias 4, Dias 6, and other five open clusters using ground-based and Gaia DR2 data [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 481( 3): 3887-3901.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/sty2341
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES

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      LAGIOIA, E. P et al. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, v. 475, n. 3, p. 4088-4103, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty083. Acesso em: 07 out. 2024.
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      Lagioia, E. P., Milone, A. P., Marino, A. F., Cassisi, S., Aparicio, A. J., Piotto, G., et al. (2018). The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, 475( 3), 4088-4103. doi:10.1093/mnras/sty083
    • NLM

      Lagioia EP, Milone AP, Marino AF, Cassisi S, Aparicio AJ, Piotto G, Anderson J, Barbuy BLS. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 4088-4103.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/sty083
    • Vancouver

      Lagioia EP, Milone AP, Marino AF, Cassisi S, Aparicio AJ, Piotto G, Anderson J, Barbuy BLS. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 4088-4103.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/sty083
  • 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: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 07 out. 2024.
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      Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
    • NLM

      Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 out. 07 ] 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. 07 ] Available from: https://doi.org/10.3847/1538-4357/aad190
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

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      BEDELL, Megan et al. The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, v. 865, n. 1, p. 68-1/68-13, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad908. Acesso em: 07 out. 2024.
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      Bedell, M., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., Asplund, M., et al. (2018). The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, 865( 1), 68-1/68-13. doi:10.3847/1538-4357/aad908
    • NLM

      Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 out. 07 ] 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. 07 ] Available from: https://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: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 07 out. 2024.
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      Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
    • NLM

      Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 out. 07 ] 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. 07 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES

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      CAIN, Madelyn et al. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, v. 864, n. 1, p. 43-1/43-12, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 07 out. 2024.
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      Cain, M., Frebel, A., Gull, M., Ji, A. P., Placco, V. M., Beers, T. C., et al. (2018). The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, 864( 1), 43-1/43-12. doi:10.3847/1538-4357/aad37d
    • NLM

      Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 out. 07 ] 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. 07 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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      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: 07 out. 2024.
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      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 out. 07 ] 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 out. 07 ] Available from: https://doi.org/10.1093/mnras/stx2199
  • Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      FISHLOCK, C. K et al. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 466, p. 4672-4682, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx047. Acesso em: 07 out. 2024.
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      Fishlock, C. K., Yong, D., Karakas, A. I., Alves-Brito, A., Moreno, J. L. M., Nissen, P. E., et al. (2017). Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 466, 4672-4682. doi:10.1093/mnras/stx047
    • NLM

      Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 out. 07 ] 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 out. 07 ] Available from: https://doi.org/10.1093/mnras/stx047
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: INSTRUMENTAÇÃO (ASTRONOMIA), ABUNDÂNCIA ESTELAR

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      MILONE, A. P et al. The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters – IX. The Atlas of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, v. 464, p. 3636-3656, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2531. Acesso em: 07 out. 2024.
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      Milone, A. P., Piotto, G., Renzini, A., Marino, A. F., & Barbuy, B. L. S. (2017). The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters – IX. The Atlas of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, 464, 3636-3656. doi:10.1093/mnras/stw2531
    • NLM

      Milone AP, Piotto G, Renzini A, Marino AF, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters – IX. The Atlas of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 464 3636-3656.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw2531
    • Vancouver

      Milone AP, Piotto G, Renzini A, Marino AF, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters – IX. The Atlas of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 464 3636-3656.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw2531
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: GALÁXIAS ELÍPTICAS, DINÂMICA DAS GALÁXIAS

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      CORTESI, Arianna et al. The SLUGGS survey: chromodynamical modelling of the lenticular galaxy NGC 1023. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2611-2621, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2753. Acesso em: 07 out. 2024.
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      Cortesi, A., Santos, A. L. C., Pota, V., Foster, C., Coccato, L., Oliveira, C. M. de, et al. (2016). The SLUGGS survey: chromodynamical modelling of the lenticular galaxy NGC 1023. Monthly Notices of the Royal Astronomical Society, 456, 2611-2621. doi:10.1093/mnras/stv2753
    • NLM

      Cortesi A, Santos ALC, Pota V, Foster C, Coccato L, Oliveira CM de, Forbes DA, Merrifield MM, Bamford SP, Romanowsky AJ, Brodie JP, Kartha SS, Alabi AB, Proctor RN, Almeida A. The SLUGGS survey: chromodynamical modelling of the lenticular galaxy NGC 1023 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2611-2621.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stv2753
    • Vancouver

      Cortesi A, Santos ALC, Pota V, Foster C, Coccato L, Oliveira CM de, Forbes DA, Merrifield MM, Bamford SP, Romanowsky AJ, Brodie JP, Kartha SS, Alabi AB, Proctor RN, Almeida A. The SLUGGS survey: chromodynamical modelling of the lenticular galaxy NGC 1023 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2611-2621.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stv2753
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      LIU, F et al. The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, v. 457, p. 3934-3948, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw247. Acesso em: 07 out. 2024.
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      Liu, F., Yong, D., Asplund, M., Ramírez, I., & Moreno, J. L. M. (2016). The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, 457, 3934-3948. doi:10.1093/mnras/stw247
    • NLM

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw247
    • Vancouver

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw247
  • Source: Atmospheric Environment. Unidade: IAG

    Subjects: POLUIÇÃO ATMOSFÉRICA, QUALIDADE DO AR, ÁREAS METROPOLITANAS

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    • ABNT

      KUMAR, Prashant et al. New directions: from biofuels to wood stoves: the modern and ancient air quality challenges in the megacity of São Paulo. Atmospheric Environment, v. 140, p. 364-369, 2016Tradução . . Disponível em: https://doi.org/10.1016/j.atmosenv.2016.05.059. Acesso em: 07 out. 2024.
    • APA

      Kumar, P., Andrade, M. de F., Ynoue, R. Y., Fornaro, A., Freitas, E. D. de, Martins, J., et al. (2016). New directions: from biofuels to wood stoves: the modern and ancient air quality challenges in the megacity of São Paulo. Atmospheric Environment, 140, 364-369. doi:10.1016/j.atmosenv.2016.05.059
    • NLM

      Kumar P, Andrade M de F, Ynoue RY, Fornaro A, Freitas ED de, Martins J, Martins LD, Albuquerque T, Zhang Y, Morawska L. New directions: from biofuels to wood stoves: the modern and ancient air quality challenges in the megacity of São Paulo [Internet]. Atmospheric Environment. 2016 ; 140 364-369.[citado 2024 out. 07 ] Available from: https://doi.org/10.1016/j.atmosenv.2016.05.059
    • Vancouver

      Kumar P, Andrade M de F, Ynoue RY, Fornaro A, Freitas ED de, Martins J, Martins LD, Albuquerque T, Zhang Y, Morawska L. New directions: from biofuels to wood stoves: the modern and ancient air quality challenges in the megacity of São Paulo [Internet]. Atmospheric Environment. 2016 ; 140 364-369.[citado 2024 out. 07 ] Available from: https://doi.org/10.1016/j.atmosenv.2016.05.059
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      LIU, F et al. The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2636-2646, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2821. Acesso em: 07 out. 2024.
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      Liu, F., Yong, D., Asplund, M., Ramírez, I., Moreno, J. L. M., Gustafsson, B., et al. (2016). The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, 456, 2636-2646. doi:10.1093/mnras/stv2821
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      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stv2821
    • Vancouver

      Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stv2821
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR

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      YONG, David et al. GRACES observations of young [α/Fe]-rich stars. Monthly Notices of the Royal Astronomical Society, v. 459, p. 487-495, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw676. Acesso em: 07 out. 2024.
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      Yong, D., Casagrande, L., Venn, K. A., Chené, A. -N., Keown, J., Malo, L., et al. (2016). GRACES observations of young [α/Fe]-rich stars. Monthly Notices of the Royal Astronomical Society, 459, 487-495. doi:10.1093/mnras/stw676
    • NLM

      Yong D, Casagrande L, Venn KA, Chené A-N, Keown J, Malo L, Martioli E, Moreno JLM. GRACES observations of young [α/Fe]-rich stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 459 487-495.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw676
    • Vancouver

      Yong D, Casagrande L, Venn KA, Chené A-N, Keown J, Malo L, Martioli E, Moreno JLM. GRACES observations of young [α/Fe]-rich stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 459 487-495.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw676
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      ASPLUND, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, v. 463, p. 696-704, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 07 out. 2024.
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      Asplund, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 463, 696-704. doi:10.1093/mnras/stw2045
    • NLM

      Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw2045
    • Vancouver

      Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw2045
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: ABUNDÂNCIA ESTELAR

    Acesso à fonteAcesso à fonteDOIHow to cite
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    • ABNT

      LIU, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 07 out. 2024.
    • APA

      Liu, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stw2045
    • NLM

      Liu F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw2045
    • Vancouver

      Liu F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2024 out. 07 ] Available from: https://doi.org/10.1093/mnras/stw2045

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