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  • Trabalho de evento

    The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk (2017)

    Mollá, Mercedes; Calvichia, Oscar; Costa, Roberto Dell'Aglio Dias da; Maciel, Walter Junqueira; Gibsaon, Brad; Diáz, Angeles I

    Source: Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. Conference titles: IAU SYMPOSIUM. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA)

    Acesso à fonteAcesso à fonteDOIHow to cite
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    • ABNT

      MOLLÁ, Mercedes et al. The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317001697. Acesso em: 04 jul. 2024.

    • APA

      Mollá, M., Calvichia, O., Costa, R. D. 'A. D. da, Maciel, W. J., Gibsaon, B., & Diáz, A. I. (2017). The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk. In Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317001697

    • NLM

      Mollá M, Calvichia O, Costa RD'AD da, Maciel WJ, Gibsaon B, Diáz AI. The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk [Internet]. Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. 2017 ;[citado 2024 jul. 04 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317001697

    • Vancouver

      Mollá M, Calvichia O, Costa RD'AD da, Maciel WJ, Gibsaon B, Diáz AI. The evolution of the oxygen abundance radial gradient in the Milky Way Galaxy disk [Internet]. Planetary nebulae: multi-wavelength probes of stellar and galactic evolution : proceedings of the 323rd Symposium of the International Astronomical Union held in Beijing, China, October 1-14, 2016. 2017 ;[citado 2024 jul. 04 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317001697

  • Trabalho de evento

    Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations (2017)

    Guerrero, G; Smolarkiewicz, P. K; Gouveia dal Pino, Elisabete Maria de; Kososichev, A. G; Zaire, B; Mansour, N. N

    Source: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Conference titles: IAU SYMPOSIUM. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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

    • ABNT

      GUERRERO, G et al. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982. Acesso em: 04 jul. 2024.

    • APA

      Guerrero, G., Smolarkiewicz, P. K., Gouveia dal Pino, E. M. de, Kososichev, A. G., Zaire, B., & Mansour, N. N. (2017). Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations. In Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317003982

    • NLM

      Guerrero G, Smolarkiewicz PK, Gouveia dal Pino EM de, Kososichev AG, Zaire B, Mansour NN. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jul. 04 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982

    • Vancouver

      Guerrero G, Smolarkiewicz PK, Gouveia dal Pino EM de, Kososichev AG, Zaire B, Mansour NN. Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 jul. 04 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003982
  • 1

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