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Filtros : "MORENO, JORGE LUIS MELENDEZ" "Galarza, Jhon J. Yana" Limpar

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  • Artigo de periodico

    How Magnetic Activity Alters What We Learn from Stellar Spectra (2020)

    Spina, Lorenzo ; Moreno, Jorge Luis Meléndez ; Galarza, Jhon J. Yana

    Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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

    • ABNT

      SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e GALARZA, Jhon J. Yana. How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab8bd7. Acesso em: 15 out. 2024.

    • APA

      Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2020). How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/ab8bd7

    • NLM

      Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7

    • Vancouver

      Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 out. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7

  • Artigo de periodico

    The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun (2020)

    Lorenzo-Oliveira, Diego ; Moreno, Jorge Luis Meléndez ; Ponte, Geisa ; Galarza, Jhon J. Yana

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

    Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS

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

    • ABNT

      LORENZO-OLIVEIRA, Diego et al. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun. Monthly Notices of the Royal Astronomical Society Letters, v. 495, p. L61-L65, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2917. Acesso em: 15 out. 2024.

    • APA

      Lorenzo-Oliveira, D., Moreno, J. L. M., Ponte, G., & Galarza, J. J. Y. (2020). The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun. Monthly Notices of the Royal Astronomical Society Letters, 495, L61-L65. doi:10.1093/mnras/staa2917

    • NLM

      Lorenzo-Oliveira D, Moreno JLM, Ponte G, Galarza JJY. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2020 ; 495 L61-L65.[citado 2024 out. 15 ] Available from: https://doi.org/10.1093/mnras/staa2917

    • Vancouver

      Lorenzo-Oliveira D, Moreno JLM, Ponte G, Galarza JJY. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2020 ; 495 L61-L65.[citado 2024 out. 15 ] Available from: https://doi.org/10.1093/mnras/staa2917
  • 1

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