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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ATIVIDADE ESTELAR, VELOCIDADE

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    • ABNT

      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: 27 abr. 2024.
    • APA

      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
    • NLM

      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 abr. 27 ] 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 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201525748
  • Source: The Astronomical Journal. Unidade: IAG

    Subjects: ESTRELAS, POPULAÇÕES ESTELARES

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    • ABNT

      PIOTTO, G et al. The Hubble Space Telescope UV legacy survey of galactic globular clusters: I. Overview of the project and detection of multiple stellar populations. The Astronomical Journal, v. 149, p. 91/1-91/28, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-6256/149/3/91. Acesso em: 27 abr. 2024.
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      Piotto, G., Milone, A. P., Bedin, L. R., & Barbuy, B. L. S. (2015). The Hubble Space Telescope UV legacy survey of galactic globular clusters: I. Overview of the project and detection of multiple stellar populations. The Astronomical Journal, 149, 91/1-91/28. doi:10.1088/0004-6256/149/3/91
    • NLM

      Piotto G, Milone AP, Bedin LR, Barbuy BLS. The Hubble Space Telescope UV legacy survey of galactic globular clusters: I. Overview of the project and detection of multiple stellar populations [Internet]. The Astronomical Journal. 2015 ; 149 91/1-91/28.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-6256/149/3/91
    • Vancouver

      Piotto G, Milone AP, Bedin LR, Barbuy BLS. The Hubble Space Telescope UV legacy survey of galactic globular clusters: I. Overview of the project and detection of multiple stellar populations [Internet]. The Astronomical Journal. 2015 ; 149 91/1-91/28.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-6256/149/3/91
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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    • ABNT

      BEDELL, Megan et al. Stellar chemical abundances: in pursuit of the highest achievable precision. The Astrophysical Journal, v. 795, p. 23/1-23/14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/795/1/23. Acesso em: 27 abr. 2024.
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      Bedell, M., Moreno, J. L. M., Bean, J. L., Ramírez, I., Leite, P., & Asplund, M. (2014). Stellar chemical abundances: in pursuit of the highest achievable precision. The Astrophysical Journal, 795, 23/1-23/14. doi:10.1088/0004-637X/795/1/23
    • NLM

      Bedell M, Moreno JLM, Bean JL, Ramírez I, Leite P, Asplund M. Stellar chemical abundances: in pursuit of the highest achievable precision [Internet]. The Astrophysical Journal. 2014 ; 795 23/1-23/14.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/795/1/23
    • Vancouver

      Bedell M, Moreno JLM, Bean JL, Ramírez I, Leite P, Asplund M. Stellar chemical abundances: in pursuit of the highest achievable precision [Internet]. The Astrophysical Journal. 2014 ; 795 23/1-23/14.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/795/1/23
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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    • ABNT

      TUCCI MAIA, M et al. Shallow extra mixing in solar twins inferred from Be abundances. Astronomy & Astrophysics, v. 576, p. L10/1-L10/4, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201425357. Acesso em: 27 abr. 2024.
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      Tucci Maia, M., Moreno, J. L. M., Castro, M., Asplund, M., Ramírez, I., Monroe, T. R., et al. (2015). Shallow extra mixing in solar twins inferred from Be abundances. Astronomy & Astrophysics, 576, L10/1-L10/4. doi:10.1051/0004-6361/201425357
    • NLM

      Tucci Maia M, Moreno JLM, Castro M, Asplund M, Ramírez I, Monroe TR, Nascimento Jr. J-D do, Yong D. Shallow extra mixing in solar twins inferred from Be abundances [Internet]. Astronomy & Astrophysics. 2015 ; 576 L10/1-L10/4.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201425357
    • Vancouver

      Tucci Maia M, Moreno JLM, Castro M, Asplund M, Ramírez I, Monroe TR, Nascimento Jr. J-D do, Yong D. Shallow extra mixing in solar twins inferred from Be abundances [Internet]. Astronomy & Astrophysics. 2015 ; 576 L10/1-L10/4.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201425357
  • Source: IAU Highlights of Astronomy, V. 16. Conference titles: IAU General Assembly. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, AGLOMERADOS (GALÁXIA)

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    • ABNT

      YONG, David et al. Precision chemical abundance measurements. 2015, Anais.. Cambridge: Cambridge University Press, 2015. Disponível em: https://doi.org/10.1017/S1743921314005572. Acesso em: 27 abr. 2024.
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      Yong, D., Grundahl, F., Moreno, J. L. M., & Norris, J. E. (2015). Precision chemical abundance measurements. In IAU Highlights of Astronomy, V. 16. Cambridge: Cambridge University Press. doi:10.1017/S1743921314005572
    • NLM

      Yong D, Grundahl F, Moreno JLM, Norris JE. Precision chemical abundance measurements [Internet]. IAU Highlights of Astronomy, V. 16. 2015 ;[citado 2024 abr. 27 ] Available from: https://doi.org/10.1017/S1743921314005572
    • Vancouver

      Yong D, Grundahl F, Moreno JLM, Norris JE. Precision chemical abundance measurements [Internet]. IAU Highlights of Astronomy, V. 16. 2015 ;[citado 2024 abr. 27 ] Available from: https://doi.org/10.1017/S1743921314005572
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: DINÂMICA DA GALÁXIA, ESTRUTURA DA GALÁXIA, ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES

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      BEERS, Timothy C et al. Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy. The Astrophysical Journal, v. 794, p. 58/1-58/19, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/794/1/58. Acesso em: 27 abr. 2024.
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      Beers, T. C., Norris, J. E., Placco, V. M., Lee, Y. S., Rossi, S. C. F., Carollo, D., & Masseron, T. (2014). Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy. The Astrophysical Journal, 794, 58/1-58/19. doi:10.1088/0004-637X/794/1/58
    • NLM

      Beers TC, Norris JE, Placco VM, Lee YS, Rossi SCF, Carollo D, Masseron T. Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy [Internet]. The Astrophysical Journal. 2014 ; 794 58/1-58/19.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/794/1/58
    • Vancouver

      Beers TC, Norris JE, Placco VM, Lee YS, Rossi SCF, Carollo D, Masseron T. Population studies: XIII. A new analysis of the Bidelman-MacConnell "weak-metal" stars - confirmation of metal-poor stars in the thick disk of the Galaxy [Internet]. The Astrophysical Journal. 2014 ; 794 58/1-58/19.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/794/1/58
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, ESPECTROSCOPIA

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      PLACCO, Vinicius M et al. Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis. The Astrophysical Journal, v. 770, n. 2, p. 104/1-104/22, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/770/2/104. Acesso em: 27 abr. 2024.
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      Placco, V. M., Frebel, A., Beers, T. C., Karakas, A. I., Kennedy, C. R., Rossi, S. C. F., et al. (2013). Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis. The Astrophysical Journal, 770( 2), 104/1-104/22. doi:10.1088/0004-637X/770/2/104
    • NLM

      Placco VM, Frebel A, Beers TC, Karakas AI, Kennedy CR, Rossi SCF, Christlieb N, Stancliffe RJ. Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis [Internet]. The Astrophysical Journal. 2013 ; 770( 2): 104/1-104/22.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/770/2/104
    • Vancouver

      Placco VM, Frebel A, Beers TC, Karakas AI, Kennedy CR, Rossi SCF, Christlieb N, Stancliffe RJ. Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis [Internet]. The Astrophysical Journal. 2013 ; 770( 2): 104/1-104/22.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/770/2/104
  • 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: 27 abr. 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 abr. 27 ] 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 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201424172
  • 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: 27 abr. 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
    • NLM

      Ramírez I, Moreno JLM, Asplund M. Chemical signatures of planets: beyond solar-twins [Internet]. Astronomy & Astrophysics. 2014 ;561 A7/1-A7/16.[citado 2024 abr. 27 ] 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 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201322558
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), ABUNDÂNCIA ESTELAR

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      ALVES-BRITO, A et al. CNO and F abundances in the globular cluster M22 (NGC 6656). Astronomy & Astrophysics, v. 540, p. A3/1-A3/12, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118623. Acesso em: 27 abr. 2024.
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      Alves-Brito, A., Yong, D., Meléndez Moreno, J. L., Vásquez, S., & Karakas, A. I. (2012). CNO and F abundances in the globular cluster M22 (NGC 6656). Astronomy & Astrophysics, 540, A3/1-A3/12. doi:10.1051/0004-6361/201118623
    • NLM

      Alves-Brito A, Yong D, Meléndez Moreno JL, Vásquez S, Karakas AI. CNO and F abundances in the globular cluster M22 (NGC 6656) [Internet]. Astronomy & Astrophysics. 2012 ; 540 A3/1-A3/12.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201118623
    • Vancouver

      Alves-Brito A, Yong D, Meléndez Moreno JL, Vásquez S, Karakas AI. CNO and F abundances in the globular cluster M22 (NGC 6656) [Internet]. Astronomy & Astrophysics. 2012 ; 540 A3/1-A3/12.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1051/0004-6361/201118623
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, ABUNDÂNCIAS SOLARES

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      MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván e KARAKAS, Amanda I. 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging. The Astrophysical Journal, v. 791, p. 14/1-14/14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/791/1/14. Acesso em: 27 abr. 2024.
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      Moreno, J. L. M., Ramírez, I., & Karakas, A. I. (2014). 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging. The Astrophysical Journal, 791, 14/1-14/14. doi:10.1088/0004-637X/791/1/14
    • NLM

      Moreno JLM, Ramírez I, Karakas AI. 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging [Internet]. The Astrophysical Journal. 2014 ; 791 14/1-14/14.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/791/1/14
    • Vancouver

      Moreno JLM, Ramírez I, Karakas AI. 18 Sco: a solar twin rich in refractory and neutron-capture elements: implications for chemical tagging [Internet]. The Astrophysical Journal. 2014 ; 791 14/1-14/14.[citado 2024 abr. 27 ] Available from: https://doi.org/10.1088/0004-637X/791/1/14

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