Filtros : "BARBUY, BEATRIZ LEONOR SILVEIRA" "Kerber, L" Removido: "2018" Limpar

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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, NUVENS DE MAGALHÃES

    Acesso à fonteAcesso à fonteDOIHow to cite
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    • ABNT

      DIAS, B et al. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527558. Acesso em: 30 ago. 2024.
    • APA

      Dias, B., Kerber, L., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2016). SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics. doi:10.1051/0004-6361/201527558
    • NLM

      Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2024 ago. 30 ] Available from: https://doi.org/10.1051/0004-6361/201527558
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ;[citado 2024 ago. 30 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS, NUVENS DE MAGALHÃES

    Acesso à fonteDOIHow to cite
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    • ABNT

      DIAS, B et al. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, v. 591, p. A11/1-A11/16, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527558. Acesso em: 30 ago. 2024.
    • APA

      Dias, B., Kerber, L., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2016). SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, 591, A11/1-A11/16. doi:10.1051/0004-6361/201527558
    • NLM

      Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ; 591 A11/1-A11/16.[citado 2024 ago. 30 ] Available from: https://doi.org/10.1051/0004-6361/201527558
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ; 591 A11/1-A11/16.[citado 2024 ago. 30 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • 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: 30 ago. 2024.
    • 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 2024 ago. 30 ] 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 2024 ago. 30 ] Available from: https://doi.org/10.1093/mnras/stv1720
  • Source: ASP Conference Series. Conference titles: Fifty Years of Wide Field Studies in the Southern Hemisphere: Resolved Stellar Populations of the Galactic Bulge and the Magellanic Clouds. Unidade: IAG

    Subjects: POPULAÇÕES ESTELARES, NUVENS DE MAGALHÃES

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    • ABNT

      DIAS, B et al. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. 2014, Anais.. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 2014. p. 338. . Acesso em: 30 ago. 2024.
    • APA

      Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortoloni, S., & Balbinot, E. (2014). Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. In ASP Conference Series (Vol. 491, p. 338). San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
    • NLM

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortoloni S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. ASP Conference Series. 2014 ; 491 338.[citado 2024 ago. 30 ]
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortoloni S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. ASP Conference Series. 2014 ; 491 338.[citado 2024 ago. 30 ]
  • Source: Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG

    Assunto: NUVENS DE MAGALHÃES

    How to cite
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    • ABNT

      DIAS, B et al. Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 30 ago. 2024. , 2014
    • APA

      Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2014). Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. México: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
    • NLM

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 2014 ; 44 153.[citado 2024 ago. 30 ]
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Parameters for SMC clusters from CMD modeling. Revista Mexicana de Astronomía y Astrofísica. Serie de Conferencias. 2014 ; 44 153.[citado 2024 ago. 30 ]
  • 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: 30 ago. 2024.
    • 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 2024 ago. 30 ]
    • 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 2024 ago. 30 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: NUVENS DE MAGALHÃES, GALÁXIAS, ESTRELAS

    Acesso à fonteDOIHow to cite
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    • ABNT

      DIAS, B et al. Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy. Astronomy & Astrophysics, v. 520, p. A85/1-A85/17, 2010Tradução . . Disponível em: https://doi.org/10.1017/s174392131000308x. Acesso em: 30 ago. 2024.
    • APA

      Dias, B., Coelho, P., Barbuy, B. L. S., Kerber, L., & Idiart, T. E. P. (2010). Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy. Astronomy & Astrophysics, 520, A85/1-A85/17. doi:10.1017/s174392131000308x
    • NLM

      Dias B, Coelho P, Barbuy BLS, Kerber L, Idiart TEP. Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy [Internet]. Astronomy & Astrophysics. 2010 ; 520 A85/1-A85/17.[citado 2024 ago. 30 ] Available from: https://doi.org/10.1017/s174392131000308x
    • Vancouver

      Dias B, Coelho P, Barbuy BLS, Kerber L, Idiart TEP. Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy [Internet]. Astronomy & Astrophysics. 2010 ; 520 A85/1-A85/17.[citado 2024 ago. 30 ] Available from: https://doi.org/10.1017/s174392131000308x

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