Filtros : "MORENO, JORGE LUIS MELENDEZ" "The Astrophysical Journal" Removido: "Teses e dissertações" Limpar

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  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS

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    • ABNT

      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.
    • APA

      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
    • NLM

      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: The Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, ABUNDÂNCIAS SOLARES

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    • ABNT

      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: 15 out. 2024.
    • APA

      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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/791/1/14
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

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      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: 15 out. 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 out. 15 ] 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 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/795/1/23
  • Source: The Astrophysical Journal. Unidade: IAG

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

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    • ABNT

      RAMÍREZ, I e MELÉNDEZ MORENO, Jorge Luis e CHANAMÉ, J. Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters. The Astrophysical Journal, v. 757, p. 164/1-164/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/757/2/164. Acesso em: 15 out. 2024.
    • APA

      Ramírez, I., Meléndez Moreno, J. L., & Chanamé, J. (2012). Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters. The Astrophysical Journal, 757, 164/1-164/13. doi:10.1088/0004-637X/757/2/164
    • NLM

      Ramírez I, Meléndez Moreno JL, Chanamé J. Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters [Internet]. The Astrophysical Journal. 2012 ; 757 164/1-164/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/757/2/164
    • Vancouver

      Ramírez I, Meléndez Moreno JL, Chanamé J. Oxygen abundances in low- and high-'alfa' field halo stars and the discovery of two field stars born in globular clusters [Internet]. The Astrophysical Journal. 2012 ; 757 164/1-164/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/757/2/164
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, SOL, FOTOMETRIA

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    • ABNT

      CASAGRANDE, L et al. The infrared colors of the sun. The Astrophysical Journal, v. 761, p. 16/1-16/9, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/761/1/16. Acesso em: 15 out. 2024.
    • APA

      Casagrande, L., Ramírez, I., Meléndez Moreno, J. L., & Asplund, M. (2012). The infrared colors of the sun. The Astrophysical Journal, 761, 16/1-16/9. doi:10.1088/0004-637X/761/1/16
    • NLM

      Casagrande L, Ramírez I, Meléndez Moreno JL, Asplund M. The infrared colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 761 16/1-16/9.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/761/1/16
    • Vancouver

      Casagrande L, Ramírez I, Meléndez Moreno JL, Asplund M. The infrared colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 761 16/1-16/9.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/761/1/16
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, SOL, FOTOMETRIA

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      RAMÍREZ, I et al. The UBV '(RI) IND. C' colors of the sun. The Astrophysical Journal, v. 752, p. 5/1-5/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/752/1/5. Acesso em: 15 out. 2024.
    • APA

      Ramírez, I., Michel, R., Sefako, R., Maia, M. T., Schuster, W. J., van Wyk, F., et al. (2012). The UBV '(RI) IND. C' colors of the sun. The Astrophysical Journal, 752, 5/1-5/13. doi:10.1088/0004-637X/752/1/5
    • NLM

      Ramírez I, Michel R, Sefako R, Maia MT, Schuster WJ, van Wyk F, Meléndez Moreno JL, Casagrande L, Castilho BV. The UBV '(RI) IND. C' colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 752 5/1-5/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/752/1/5
    • Vancouver

      Ramírez I, Michel R, Sefako R, Maia MT, Schuster WJ, van Wyk F, Meléndez Moreno JL, Casagrande L, Castilho BV. The UBV '(RI) IND. C' colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 752 5/1-5/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/752/1/5
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS

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      RAMÍREZ, I et al. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation?. The Astrophysical Journal, v. 740, p. 76/1-76/15, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/740/2/76. Acesso em: 15 out. 2024.
    • APA

      Ramírez, I., Meléndez Moreno, J. L., Cornejo, D., Roederer, I. U., & Fish, J. R. (2011). Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? The Astrophysical Journal, 740, 76/1-76/15. doi:10.1088/0004-637X/740/2/76
    • NLM

      Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76
    • Vancouver

      Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76

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