Filtros : "ABUNDÂNCIA ESTELAR" "The Australian National University, Weston, Australia" "2014" Limpar

Filtros



Refine with date range


  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, PLANETAS

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 14 set. 2024.
    • APA

      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 set. 14 ] 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 set. 14 ] Available from: https://doi.org/10.1051/0004-6361/201322558
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, ABUNDÂNCIAS SOLARES

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • 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: 14 set. 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 set. 14 ] 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 set. 14 ] Available from: https://doi.org/10.1088/0004-637X/791/1/14
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • 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: 14 set. 2024.
    • APA

      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 set. 14 ] 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 set. 14 ] Available from: https://doi.org/10.1088/0004-637X/795/1/23
  • Source: The Astrophysical Journal. Unidade: IAG

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

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 14 set. 2024.
    • APA

      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 set. 14 ] 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 set. 14 ] Available from: https://doi.org/10.1088/0004-637X/794/1/58
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

    Acesso à fonteDOIHow to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      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: 14 set. 2024.
    • APA

      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 set. 14 ] 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 set. 14 ] Available from: https://doi.org/10.1051/0004-6361/201424172

Digital Library of Intellectual Production of Universidade de São Paulo     2012 - 2024