Filtros : "Diaz, Marcos Perez" "Brasil" Removido: "Brasil" Limpar

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

    Subjects: ESTRELAS VARIÁVEIS, POLARIZAÇÃO (ASTRONOMIA)

    Acesso à fonteDOIHow to cite
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    • ABNT

      OLIVEIRA, Alexandre S. et al. Optical observations and CYCLOPS post-shock region modelling of the polar V348 Pav. Monthly Notices of the Royal Astronomical Society, v. 489, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2445. Acesso em: 17 out. 2024.
    • APA

      Oliveira, A. S., Rodrigues, C. V., Pallares, M. S., Diaz, M. P., Belloni, D., & Silva, K. M. G. (2019). Optical observations and CYCLOPS post-shock region modelling of the polar V348 Pav. Monthly Notices of the Royal Astronomical Society, 489. doi:10.1093/mnras/stz2445
    • NLM

      Oliveira AS, Rodrigues CV, Pallares MS, Diaz MP, Belloni D, Silva KMG. Optical observations and CYCLOPS post-shock region modelling of the polar V348 Pav [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489[citado 2024 out. 17 ] Available from: https://doi.org/10.1093/mnras/stz2445
    • Vancouver

      Oliveira AS, Rodrigues CV, Pallares MS, Diaz MP, Belloni D, Silva KMG. Optical observations and CYCLOPS post-shock region modelling of the polar V348 Pav [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489[citado 2024 out. 17 ] Available from: https://doi.org/10.1093/mnras/stz2445
  • Source: New Astronomy. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ESPECTROSCOPIA

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    • ABNT

      BRUCH, Albert e DIAZ, Marcos Perez. Time resolved spectroscopy and photometry of three little known bright cataclysmic variables: LS IV -08° 3, HQ monocerotis and ST chamaeleontis. New Astronomy, v. 50, p. 109-119, 2017Tradução . . Disponível em: https://doi.org/10.1016/j.newast.2016.07.011. Acesso em: 17 out. 2024.
    • APA

      Bruch, A., & Diaz, M. P. (2017). Time resolved spectroscopy and photometry of three little known bright cataclysmic variables: LS IV -08° 3, HQ monocerotis and ST chamaeleontis. New Astronomy, 50, 109-119. doi:10.1016/j.newast.2016.07.011
    • NLM

      Bruch A, Diaz MP. Time resolved spectroscopy and photometry of three little known bright cataclysmic variables: LS IV -08° 3, HQ monocerotis and ST chamaeleontis [Internet]. New Astronomy. 2017 ;50 109-119.[citado 2024 out. 17 ] Available from: https://doi.org/10.1016/j.newast.2016.07.011
    • Vancouver

      Bruch A, Diaz MP. Time resolved spectroscopy and photometry of three little known bright cataclysmic variables: LS IV -08° 3, HQ monocerotis and ST chamaeleontis [Internet]. New Astronomy. 2017 ;50 109-119.[citado 2024 out. 17 ] Available from: https://doi.org/10.1016/j.newast.2016.07.011
  • Source: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. Unidade: IAG

    Assunto: ATMOSFERAS ESTELARES

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    • ABNT

      LEVENHAGEM, Ronaldo Savarino et al. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v. 231, n. 1, p. 1, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/aa7681. Acesso em: 17 out. 2024.
    • APA

      Levenhagem, R. S., Diaz, M. P., Coelho, P. R. T., & Hubeny, I. (2017). A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 231( 1), 1. doi:10.3847/1538-4365/aa7681
    • NLM

      Levenhagem RS, Diaz MP, Coelho PRT, Hubeny I. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2017 ;231( 1): 1.[citado 2024 out. 17 ] Available from: https://doi.org/10.3847/1538-4365/aa7681
    • Vancouver

      Levenhagem RS, Diaz MP, Coelho PRT, Hubeny I. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2017 ;231( 1): 1.[citado 2024 out. 17 ] Available from: https://doi.org/10.3847/1538-4365/aa7681

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