Filtros : "ABUNDÂNCIA ESTELAR" "PLANETAS" Removido: "Ramírez, I" Limpar

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  • 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: 01 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
    • NLM

      Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 out. 01 ] 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. 01 ] Available from: https://doi.org/10.1051/0004-6361/201629294
  • 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: 01 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
    • 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 out. 01 ] 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. 01 ] Available from: https://doi.org/10.1051/0004-6361/201527775
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

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    • 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: 01 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
    • 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 out. 01 ] 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. 01 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
  • Source: Astrophysical Journal (Online). Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, PLANETAS

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    • ABNT

      STORCHI-BERGMANN, Thaisa et al. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei. Astrophysical Journal (Online), v. 835, n. 2, p. 236, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/2/236. Acesso em: 01 out. 2024.
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      Storchi-Bergmann, T., Schimoia, J. S., Peterson, B. M., Elvis, M., Denney, K. D., Eracleous, M., & Silva, R. N. da. (2017). Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei. Astrophysical Journal (Online), 835( 2), 236. doi:10.3847/1538-4357/835/2/236
    • NLM

      Storchi-Bergmann T, Schimoia JS, Peterson BM, Elvis M, Denney KD, Eracleous M, Silva RN da. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei [Internet]. Astrophysical Journal (Online). 2017 ;835( 2): 236.[citado 2024 out. 01 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
    • Vancouver

      Storchi-Bergmann T, Schimoia JS, Peterson BM, Elvis M, Denney KD, Eracleous M, Silva RN da. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei [Internet]. Astrophysical Journal (Online). 2017 ;835( 2): 236.[citado 2024 out. 01 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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    • ABNT

      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: 01 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
    • 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 2024 out. 01 ] 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. 01 ] 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: 01 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
    • 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 2024 out. 01 ] 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. 01 ] Available from: https://doi.org/10.1051/0004-6361/201527477
  • 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: 01 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
    • 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 2024 out. 01 ] 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. 01 ] 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: 01 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
    • NLM

      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. 01 ] 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. 01 ] Available from: https://doi.org/10.1051/0004-6361/201527478
  • 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: 01 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
    • NLM

      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. 01 ] 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. 01 ] Available from: https://doi.org/10.1051/0004-6361/201424172
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES

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      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: 01 out. 2024.
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      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. 01 ] 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. 01 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: PLANETAS, ESTRELAS, ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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      SANTOS, N. C et al. Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample. Astronomy & Astrophysics, v. 538, p. A151/1-A151/6, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118276. Acesso em: 01 out. 2024.
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      Santos, N. C., Lovis, C., Meléndez Moreno, J. L., Montalto, M., Naef, D., & Pace, G. (2012). Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample. Astronomy & Astrophysics, 538, A151/1-A151/6. doi:10.1051/0004-6361/201118276
    • NLM

      Santos NC, Lovis C, Meléndez Moreno JL, Montalto M, Naef D, Pace G. Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample [Internet]. Astronomy & Astrophysics. 2012 ; 538 A151/1-A151/6.[citado 2024 out. 01 ] Available from: https://doi.org/10.1051/0004-6361/201118276
    • Vancouver

      Santos NC, Lovis C, Meléndez Moreno JL, Montalto M, Naef D, Pace G. Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample [Internet]. Astronomy & Astrophysics. 2012 ; 538 A151/1-A151/6.[citado 2024 out. 01 ] Available from: https://doi.org/10.1051/0004-6361/201118276

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