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  • 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: 02 dez. 2022.
    • 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 2022 dez. 02 ] Available from: https://doi.org/10.1093/mnras/staa2917
    • Vancouver

      Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2022 dez. 02 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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    • 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: 02 dez. 2022.
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      Carlos, M., Milone, A. de C., Moreno, J. L. M., Nascimento Júnior, J. D. do, & Castro, M. (2020). Li abundances for solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 492, 245-249. doi:10.1093/mnras/stz3504
    • NLM

      Carlos M, Milone A de C, Moreno JLM, Nascimento Júnior JD do, Castro M. Li abundances for solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492 245-249.[citado 2022 dez. 02 ] Available from: https://doi.org/10.1093/mnras/stz3504
    • Vancouver

      Carlos M, Milone A de C, Moreno JLM, Nascimento Júnior JD do, Castro M. Li abundances for solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492 245-249.[citado 2022 dez. 02 ] Available from: https://doi.org/10.1093/mnras/stz3504
  • 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: 02 dez. 2022.
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      Lorenzo-Oliveira, D., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., Lambert, D. L., & Moreno, J. L. M. (2019). Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/slz034
    • NLM

      Lorenzo-Oliveira D, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL, Moreno JLM. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2022 dez. 02 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Lorenzo-Oliveira D, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL, Moreno JLM. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2022 dez. 02 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, PLANETAS

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    • 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: 02 dez. 2022.
    • 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 2022 dez. 02 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Botelho R, Moreno JLM, Alves-Brito A, Galarza JY. Thorium in solar twins: implications for habitability in rocky planets [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482 1690-1700.[citado 2022 dez. 02 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESPECTROSCOPIA, ABUNDANCIAS SOLARES

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    • 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: 02 dez. 2022.
    • 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 2022 dez. 02 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
    • Vancouver

      Carlos M, Moreno JLM, Spina L, dos Santos LA, Bedell M, Ramirez I, Asplund M, Bean JL, Yong D, Yana Galarza J, Alves-Brito A. The Li-age correlation: the sun is unusually Li deficient for its age [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 485 4052-4059.[citado 2022 dez. 02 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • 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: 02 dez. 2022.
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      Lorenzo-Oliveira, D., Freitas, F. C., Moreno, J. L. M., & Bedell, M. (2018). The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, 619, A73. doi:10.1051/0004-6364/201629294
    • 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 2022 dez. 02 ] 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 2022 dez. 02 ] Available from: https://doi.org/10.1051/0004-6361/201629294
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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    • 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: 02 dez. 2022.
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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 2022 dez. 02 ] 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 2022 dez. 02 ] 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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    • 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:10.1093/mnras/stx047. Acesso em: 02 dez. 2022.
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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/stw3194
    • 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 2022 dez. 02 ] Available from: https://doi: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 2022 dez. 02 ] Available from: https://doi:10.1093/mnras/stx047
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      MORENO, Jorge Luiz Meléndez et al. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, v. 597, p. A34, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527775. Acesso em: 02 dez. 2022.
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      Moreno, J. L. M., Bedell, M., Bean, J. L., Mello, S. F., Galarza, J. Y., Santos, L. dos, et al. (2017). The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, 597, A34. doi:10.1051/0004-6361/201527775
    • NLM

      Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2022 dez. 02 ] 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 2022 dez. 02 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • Source: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Conference title: IAU SYMPOSIUM. Unidade: IAG

    Subjects: ATIVIDADE SOLAR, ATIVIDADE ESTELAR, ESPECTROSCOPIA

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    • 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: 02 dez. 2022.
    • 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 2022 dez. 02 ] 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 2022 dez. 02 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317004203
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

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      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: 02 dez. 2022.
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      Bedell, M., Mills, S. M., Fabrycky, D. C., Freitas, F. C., Ramírez, I., Asplund, M., 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, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D, Bean JL, Moreno JLM. 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 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
    • Vancouver

      Bedell M, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D, Bean JL, Moreno JLM. 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 2022 dez. 02 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: http://dx.doi.org/10.1051/0004-6361/201527429. Acesso em: 02 dez. 2022.
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      Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
    • NLM

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527429
    • Vancouver

      Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527429
  • 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: http://dx.doi.org/10.1093/mnras/stw247. Acesso em: 02 dez. 2022.
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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 2022 dez. 02 ] Available from: http://dx.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 2022 dez. 02 ] Available from: http://dx.doi.org/10.1093/mnras/stw247
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 590, p. A66/1-A66/8, 2016Tradução . . Disponível em: http://dx.doi.org/10.1051/0004-6361/201526643. Acesso em: 02 dez. 2022.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 590, A66/1-A66/8. doi:10.1051/0004-6361/201526643
    • NLM

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 590 A66/1-A66/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201526643
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 590 A66/1-A66/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201526643
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: SOL, ESTRELAS

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      SANTOS, Leonardo A. dos et al. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, v. 592, p. A156/1-A156/8, 2016Tradução . . Disponível em: http://dx.doi.org/10.1051/0004-6361/201628558. Acesso em: 02 dez. 2022.
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      Santos, L. A. dos, Moreno, J. L. M., Nascimento Júnior, J. D. do, Bedell, M., Ramírez, I., Bean, J. L., et al. (2016). The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, 592, A156/1-A156/8. doi:10.1051/0004-6361/201628558
    • NLM

      Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201628558
    • Vancouver

      Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201628558
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      REGGIANI, Henrique et al. First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, v. 586, p. A67/1-A67/8, 2016Tradução . . Disponível em: http://dx.doi.org/10.1051/0004-6361/201527439. Acesso em: 02 dez. 2022.
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      Reggiani, H., Moreno, J. L. M., Yong, D., Ramírez, I., & Asplund, M. (2016). First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, 586, A67/1-A67/8. doi:10.1051/0004-6361/201527439
    • NLM

      Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527439
    • Vancouver

      Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527439
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, TERRA (PLANETA), PLANETAS

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    • ABNT

      GALARZA, Jhon Yana e MORENO, Jorge Luiz Meléndez e COHEN, Judith G. Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, v. 589, p. A65/1-A65/8, 2016Tradução . . Disponível em: http://dx.doi.org/10.1051/0004-6361/201527477. Acesso em: 02 dez. 2022.
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      Galarza, J. Y., Moreno, J. L. M., & Cohen, J. G. (2016). Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, 589, A65/1-A65/8. doi:10.1051/0004-6361/201527477
    • NLM

      Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527477
    • Vancouver

      Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527477
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA

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    • ABNT

      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 02 dez. 2022.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 588, A66. doi:10.1051/0004-6361/201526643
    • NLM

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2022 dez. 02 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2022 dez. 02 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, PLANETAS

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    • ABNT

      GALARZA, Jhon Yana et al. High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, v. 589, p. A17/1-A17/8, 2016Tradução . . Disponível em: http://dx.doi.org/10.1051/0004-6361/201527912. Acesso em: 02 dez. 2022.
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      Galarza, J. Y., Moreno, J. L. M., Ramírez, I., Yong, D., Karakas, A. I., Asplund, M., & Liu, F. (2016). High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, 589, A17/1-A17/8. doi:10.1051/0004-6361/201527912
    • NLM

      Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527912
    • Vancouver

      Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2022 dez. 02 ] Available from: http://dx.doi.org/10.1051/0004-6361/201527912
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subject: ABUNDÂNCIA ESTELAR

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    • ABNT

      MORENO, Jorge Luiz Meléndez et al. 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star. Astronomy & Astrophysics, 2016Tradução . . Disponível em: https://www.aanda.org/articles/aa/abs/2016/09/aa28411-16/aa28411-16.html. Acesso em: 02 dez. 2022.
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      Moreno, J. L. M., Placco, V. M., Tucci-Maia, M., Ramírez, I., Li, T. S., & Perez, G. (2016). 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star. Astronomy & Astrophysics. doi:10.1051/0004-6361/201527456
    • NLM

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2022 dez. 02 ] Available from: https://www.aanda.org/articles/aa/abs/2016/09/aa28411-16/aa28411-16.html
    • Vancouver

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2 MASS J18082002-5104378: The brightest (V = 11.9) ultra metal-poor star [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2022 dez. 02 ] Available from: https://www.aanda.org/articles/aa/abs/2016/09/aa28411-16/aa28411-16.html

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