Filtros : "Balbinot, E" Removido: "2014" Limpar

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

    Subjects: NUVENS DE MAGALHÃES, AGLOMERADOS DE GALÁXIAS

    Acesso à fonteDOIHow to cite
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    • ABNT

      BICA, E et al. Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses. Monthly Notices of the Royal Astronomical Society, v. 453, p. 3190-3102, 2015Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv1720. Acesso em: 15 out. 2025.
    • APA

      Bica, E., Santiago, B., Bonatto, C., Garcia-Dias, R., Kerber, L., Dias, B., et al. (2015). Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses. Monthly Notices of the Royal Astronomical Society, 453, 3190-3102. doi:10.1093/mnras/stv1720
    • NLM

      Bica E, Santiago B, Bonatto C, Garcia-Dias R, Kerber L, Dias B, Barbuy BLS, Balbinot E. Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 453 3190-3102.[citado 2025 out. 15 ] Available from: https://doi.org/10.1093/mnras/stv1720
    • Vancouver

      Bica E, Santiago B, Bonatto C, Garcia-Dias R, Kerber L, Dias B, Barbuy BLS, Balbinot E. Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses [Internet]. Monthly Notices of the Royal Astronomical Society. 2015 ; 453 3190-3102.[citado 2025 out. 15 ] Available from: https://doi.org/10.1093/mnras/stv1720
  • Source: LARIM 2013: Abstract Book. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG

    Subjects: NUVENS DE MAGALHÃES, ESTRELAS

    How to cite
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    • ABNT

      DIAS, B et al. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 15 out. 2025.
    • APA

      Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2013). Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
    • NLM

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. LARIM 2013: Abstract Book. 2013 ;[citado 2025 out. 15 ]
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. LARIM 2013: Abstract Book. 2013 ;[citado 2025 out. 15 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ESTRELAS, NUVENS DE MAGALHÃES

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

      BALBINOT, E et al. Probing the Large Magellanic Cloud age gap at intermediate cluster masses. Monthly Notices of the Royal Astronomical Society, v. 404, n. 3, p. 1625-1632, 2010Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2010.16390.x. Acesso em: 15 out. 2025.
    • APA

      Balbinot, E., Santiago, B. X., Kerber, L. O., Barbuy, B. L. S., & Dias, B. M. S. (2010). Probing the Large Magellanic Cloud age gap at intermediate cluster masses. Monthly Notices of the Royal Astronomical Society, 404( 3), 1625-1632. doi:10.1111/j.1365-2966.2010.16390.x
    • NLM

      Balbinot E, Santiago BX, Kerber LO, Barbuy BLS, Dias BMS. Probing the Large Magellanic Cloud age gap at intermediate cluster masses [Internet]. Monthly Notices of the Royal Astronomical Society. 2010 ; 404( 3): 1625-1632.[citado 2025 out. 15 ] Available from: https://doi.org/10.1111/j.1365-2966.2010.16390.x
    • Vancouver

      Balbinot E, Santiago BX, Kerber LO, Barbuy BLS, Dias BMS. Probing the Large Magellanic Cloud age gap at intermediate cluster masses [Internet]. Monthly Notices of the Royal Astronomical Society. 2010 ; 404( 3): 1625-1632.[citado 2025 out. 15 ] Available from: https://doi.org/10.1111/j.1365-2966.2010.16390.x

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