Filtros : "MORENO, JORGE LUIS MELENDEZ" "PLANETAS" Removido: "Holanda" Limpar

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  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDANCIA ESTELAR, PLANETAS

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      BOTELHO, Roberto et al. Thorium in solar twins: implications for habitability in rocky planets. Monthly Notices of the Royal Astronomical Society, v. 482, p. 1690-1700, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 15 out. 2024.
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      Botelho, R., Moreno, J. L. M., Alves-Brito, A., & Galarza, J. Y. (2019). Thorium in solar twins: implications for habitability in rocky planets. Monthly Notices of the Royal Astronomical Society, 482, 1690-1700. doi:10.1093/mnras/sty2791
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      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 out. 15 ] 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 out. 15 ] 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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      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.
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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:10.1051/0004-6361/201629294
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      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
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR

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      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: 15 out. 2024.
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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
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      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • 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: 15 out. 2024.
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      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
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      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 out. 15 ] 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 out. 15 ] 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: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 15 out. 2024.
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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
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      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 2024 out. 15 ] Available from: https://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 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201527429
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      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: https://doi.org/10.1051/0004-6361/201527477. Acesso em: 15 out. 2024.
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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
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      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 2024 out. 15 ] Available from: https://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 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201527477
  • 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: 15 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
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      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. 15 ] 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. 15 ] Available from: https://doi.org/10.1093/mnras/stw247
  • 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: 15 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. 15 ] 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. 15 ] Available from: https://doi.org/10.1093/mnras/stv2821
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, PLANETAS

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      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: https://doi.org/10.1051/0004-6361/201527912. Acesso em: 15 out. 2024.
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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
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      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 2024 out. 15 ] Available from: https://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 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201527912
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, PLANETAS

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      CARLOS, Marília e NISSEN, Poul E e MORENO, Jorge Luiz Meléndez. Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, v. 587, p. A100/1-A100/6, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527478. Acesso em: 15 out. 2024.
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      Carlos, M., Nissen, P. E., & Moreno, J. L. M. (2016). Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, 587, A100/1-A100/6. doi:10.1051/0004-6361/201527478
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      Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201527478
    • Vancouver

      Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201527478
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ATIVIDADE ESTELAR, VELOCIDADE

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      BEDELL, M et al. The solar twin planet search: II. A Jupiter twin around a solar twin. Astronomy & Astrophysics, v. 581, p. A34/1-A34/7, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525748. Acesso em: 15 out. 2024.
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      Bedell, M., Moreno, J. L. M., Bean, J. L., Ramírez, I., Asplund, M., Alves-Brito, A., et al. (2015). The solar twin planet search: II. A Jupiter twin around a solar twin. Astronomy & Astrophysics, 581, A34/1-A34/7. doi:10.1051/0004-6361/201525748
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      Bedell M, Moreno JLM, Bean JL, Ramírez I, Asplund M, Alves-Brito A, Casagrande L, Dreizler S, Monroe T, Spina L, Tucci Maia M. The solar twin planet search: II. A Jupiter twin around a solar twin [Internet]. Astronomy & Astrophysics. 2015 ; 581 A34/1-A34/7.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201525748
    • Vancouver

      Bedell M, Moreno JLM, Bean JL, Ramírez I, Asplund M, Alves-Brito A, Casagrande L, Dreizler S, Monroe T, Spina L, Tucci Maia M. The solar twin planet search: II. A Jupiter twin around a solar twin [Internet]. Astronomy & Astrophysics. 2015 ; 581 A34/1-A34/7.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201525748
  • Source: The Messenger. Unidade: IAG

    Subjects: PLANETAS, ASTROFÍSICA ESTELAR, ESTRELAS

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      MORENO, Jorge Luiz Meléndez et al. Using solar twins to explore the planet–star connection with unparallelled precision. The Messenger, v. 161, p. 28-31, 2015Tradução . . Disponível em: http://www.eso.org/sci/publications/messenger/archive/no.161-sep15/messenger-no161-28-31.pdf. Acesso em: 15 out. 2024.
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      Moreno, J. L. M., Bean, J. L., Bedell, M., Ramírez, I., Asplund, M., Dreizler, S., et al. (2015). Using solar twins to explore the planet–star connection with unparallelled precision. The Messenger, 161, 28-31. Recuperado de http://www.eso.org/sci/publications/messenger/archive/no.161-sep15/messenger-no161-28-31.pdf
    • NLM

      Moreno JLM, Bean JL, Bedell M, Ramírez I, Asplund M, Dreizler S, Alves-Brito A, Spina L, Casagrande L, Monroe TW, Maia MT, Freitas F. Using solar twins to explore the planet–star connection with unparallelled precision [Internet]. The Messenger. 2015 ; 161 28-31.[citado 2024 out. 15 ] Available from: http://www.eso.org/sci/publications/messenger/archive/no.161-sep15/messenger-no161-28-31.pdf
    • Vancouver

      Moreno JLM, Bean JL, Bedell M, Ramírez I, Asplund M, Dreizler S, Alves-Brito A, Spina L, Casagrande L, Monroe TW, Maia MT, Freitas F. Using solar twins to explore the planet–star connection with unparallelled precision [Internet]. The Messenger. 2015 ; 161 28-31.[citado 2024 out. 15 ] Available from: http://www.eso.org/sci/publications/messenger/archive/no.161-sep15/messenger-no161-28-31.pdf
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS

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      RAMÍREZ, I et al. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, v. 808, p. 13/1-13/14, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/13. Acesso em: 15 out. 2024.
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      Ramírez, I., Khanal, S., Aleo, P., Sobotka, A., Liu, F., Casagrande, L., et al. (2015). The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, 808, 13/1-13/14. doi:10.1088/0004-637X/808/1/13
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      Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
    • Vancouver

      Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
  • Source: Caderno de Resumos. Conference titles: Simpósio de Iniciação Científica do IAG-USP. Unidade: IAG

    Subjects: PLANETAS, ATIVIDADE ESTELAR

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      FREITAS, Fabrício Catani de. A descoberta de novos planetas com dados do HARPS/ESO. 2014, Anais.. São Paulo: IAG-USP, 2014. . Acesso em: 15 out. 2024.
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      Freitas, F. C. de. (2014). A descoberta de novos planetas com dados do HARPS/ESO. In Caderno de Resumos. São Paulo: IAG-USP.
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      Freitas FC de. A descoberta de novos planetas com dados do HARPS/ESO. Caderno de Resumos. 2014 ;[citado 2024 out. 15 ]
    • Vancouver

      Freitas FC de. A descoberta de novos planetas com dados do HARPS/ESO. Caderno de Resumos. 2014 ;[citado 2024 out. 15 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, PLANETAS

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      RAMÍREZ, I e MORENO, Jorge Luiz Meléndez e ASPLUND, M. Chemical signatures of planets: beyond solar-twins. Astronomy & Astrophysics, v. 561, p. A7/1-A7/16, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322558. Acesso em: 15 out. 2024.
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      Ramírez, I., Moreno, J. L. M., & Asplund, M. (2014). Chemical signatures of planets: beyond solar-twins. Astronomy & Astrophysics, 561, A7/1-A7/16. doi:10.1051/0004-6361/201322558
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      Ramírez I, Moreno JLM, Asplund M. Chemical signatures of planets: beyond solar-twins [Internet]. Astronomy & Astrophysics. 2014 ;561 A7/1-A7/16.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201322558
    • Vancouver

      Ramírez I, Moreno JLM, Asplund M. Chemical signatures of planets: beyond solar-twins [Internet]. Astronomy & Astrophysics. 2014 ;561 A7/1-A7/16.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201322558
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: SOL, ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS

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      MORENO, Jorge Luiz Meléndez et al. HIP 114328: a new refractory-poor and Li-poor solar twin. Astronomy & Astrophysics, v. 567, p. L3/1-L3/5, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424172. Acesso em: 15 out. 2024.
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      Moreno, J. L. M., Schirbel, L., Monroe, T. W. R., Yong, D., Ramírez, I., & Asplund, M. (2014). HIP 114328: a new refractory-poor and Li-poor solar twin. Astronomy & Astrophysics, 567, L3/1-L3/5. doi:10.1051/0004-6361/201424172
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      Moreno JLM, Schirbel L, Monroe TWR, Yong D, Ramírez I, Asplund M. HIP 114328: a new refractory-poor and Li-poor solar twin [Internet]. Astronomy & Astrophysics. 2014 ; 567 L3/1-L3/5.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201424172
    • Vancouver

      Moreno JLM, Schirbel L, Monroe TWR, Yong D, Ramírez I, Asplund M. HIP 114328: a new refractory-poor and Li-poor solar twin [Internet]. Astronomy & Astrophysics. 2014 ; 567 L3/1-L3/5.[citado 2024 out. 15 ] Available from: https://doi.org/10.1051/0004-6361/201424172
  • Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, FORMAÇÃO DO SISTEMA SOLAR, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS BINÁRIAS

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      LIU, F et al. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, v. 442, p. L51-L55, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slu055. Acesso em: 15 out. 2024.
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      Liu, F., Asplund, M., Ramírez, I., Yong, D., & Moreno, J. L. M. (2014). A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, 442, L51-L55. doi:10.1093/mnrasl/slu055
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      Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 out. 15 ] Available from: https://doi.org/10.1093/mnrasl/slu055
    • Vancouver

      Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 out. 15 ] Available from: https://doi.org/10.1093/mnrasl/slu055
  • Source: LARIM 2013: Abstract Book. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG

    Subjects: PLANETAS, INSTRUMENTAÇÃO (ASTRONOMIA)

    How to cite
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    • ABNT

      FREITAS, C. F e MORENO, Jorge Luiz Meléndez. Finding new planets around solar twins using the HARPS/ESO spectrograph. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 15 out. 2024.
    • APA

      Freitas, C. F., & Moreno, J. L. M. (2013). Finding new planets around solar twins using the HARPS/ESO spectrograph. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
    • NLM

      Freitas CF, Moreno JLM. Finding new planets around solar twins using the HARPS/ESO spectrograph. LARIM 2013: Abstract Book. 2013 ;[citado 2024 out. 15 ]
    • Vancouver

      Freitas CF, Moreno JLM. Finding new planets around solar twins using the HARPS/ESO spectrograph. LARIM 2013: Abstract Book. 2013 ;[citado 2024 out. 15 ]
  • Unidade: IAG

    Subjects: TERRA (PLANETA), PLANETAS

    Acesso à fonteHow to cite
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    • ABNT

      MORENO, Jorge Luiz Meléndez. Cientistas descobrem planeta semalhante à Terra. . São Paulo: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Disponível em: http://br.noticias.yahoo.com/cientistas-descobrem-planeta-semelhante-à-terra-113000362.html. Acesso em: 15 out. 2024. , 2013
    • APA

      Moreno, J. L. M. (2013). Cientistas descobrem planeta semalhante à Terra. São Paulo: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Recuperado de http://br.noticias.yahoo.com/cientistas-descobrem-planeta-semelhante-à-terra-113000362.html
    • NLM

      Moreno JLM. Cientistas descobrem planeta semalhante à Terra [Internet]. 2013 ;[citado 2024 out. 15 ] Available from: http://br.noticias.yahoo.com/cientistas-descobrem-planeta-semelhante-à-terra-113000362.html
    • Vancouver

      Moreno JLM. Cientistas descobrem planeta semalhante à Terra [Internet]. 2013 ;[citado 2024 out. 15 ] Available from: http://br.noticias.yahoo.com/cientistas-descobrem-planeta-semelhante-à-terra-113000362.html
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

    Acesso à fonteDOIHow to cite
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    • ABNT

      MONROE, Tala Wanda R et al. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun. The Astrophysical Journal Letters, v. 774, p. L32/1-L32/6, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/774/2/L32. Acesso em: 15 out. 2024.
    • APA

      Monroe, T. W. R., Moreno, J. L. M., Maia, M. T., & Freitas, F. C. (2013). High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun. The Astrophysical Journal Letters, 774, L32/1-L32/6. doi:10.1088/2041-8205/774/2/L32
    • NLM

      Monroe TWR, Moreno JLM, Maia MT, Freitas FC. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun [Internet]. The Astrophysical Journal Letters. 2013 ; 774 L32/1-L32/6.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
    • Vancouver

      Monroe TWR, Moreno JLM, Maia MT, Freitas FC. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun [Internet]. The Astrophysical Journal Letters. 2013 ; 774 L32/1-L32/6.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32

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