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Artigo de periodico
High-resolution spectral line indices useful for the analysis of stellar populations (2020)
Rodriguez-Merino, Lino Hector ; Mayya, Y. D ; Coelho, Paula Rodrigues Teixeira
Source: The Astrophysical Journal Letters. Unidade: IAG
Assunto: POPULAÇÕES ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RODRIGUEZ-MERINO, Lino Hector e MAYYA, Y. D e COELHO, Paula Rodrigues Teixeira. High-resolution spectral line indices useful for the analysis of stellar populations. The Astrophysical Journal Letters, v. 889, p. . L31, 2020Tradução . . Disponível em: https://doi.org/10.3847/2041-8213/ab6d64. Acesso em: 03 out. 2024.
APA
Rodriguez-Merino, L. H., Mayya, Y. D., & Coelho, P. R. T. (2020). High-resolution spectral line indices useful for the analysis of stellar populations. The Astrophysical Journal Letters, 889, . L31. doi:10.3847/2041-8213/ab6d64
NLM
Rodriguez-Merino LH, Mayya YD, Coelho PRT. High-resolution spectral line indices useful for the analysis of stellar populations [Internet]. The Astrophysical Journal Letters. 2020 ; 889 . L31.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/2041-8213/ab6d64
Vancouver
Rodriguez-Merino LH, Mayya YD, Coelho PRT. High-resolution spectral line indices useful for the analysis of stellar populations [Internet]. The Astrophysical Journal Letters. 2020 ; 889 . L31.[citado 2024 out. 03 ] Available from: https://doi.org/10.3847/2041-8213/ab6d64
Artigo de periodico
To use or not to use synthetic stellar spectra in population synthesis models? (2020)
Coelho, Paula Rodrigues Teixeira ; Bruzual, Gustavo ; Gonçalves, T S; Charlot, Stéphane
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: GALÁXIAS, ATMOSFERAS ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
COELHO, Paula Rodrigues Teixeira et al. To use or not to use synthetic stellar spectra in population synthesis models?. Monthly Notices of the Royal Astronomical Society, v. 491, n. 2, p. 2025-2042, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz3609. Acesso em: 03 out. 2024.
APA
Coelho, P. R. T., Bruzual, G., Gonçalves, T. S., & Charlot, S. (2020). To use or not to use synthetic stellar spectra in population synthesis models? Monthly Notices of the Royal Astronomical Society, 491( 2), 2025-2042. doi:10.1093/mnras/stz3609
NLM
Coelho PRT, Bruzual G, Gonçalves TS, Charlot S. To use or not to use synthetic stellar spectra in population synthesis models? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 2): 2025-2042.[citado 2024 out. 03 ] Available from: https://doi.org/10.1093/mnras/stz3609
Vancouver
Coelho PRT, Bruzual G, Gonçalves TS, Charlot S. To use or not to use synthetic stellar spectra in population synthesis models? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 2): 2025-2042.[citado 2024 out. 03 ] Available from: https://doi.org/10.1093/mnras/stz3609
Artigo de periodico
Abundance patterns in early-type galaxies: is there a "knee" in the [Fe/H] vs. ['alfa'/Fe] relation? (2015)
Walcher, C. J; Coelho, Paula Rodrigues Teixeira; Gallazzi, A; Bruzual, G; Charlot, S; Chiappini, C
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIAS (ASTRONOMIA), GALÁXIAS, GALÁXIAS ELÍPTICAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
WALCHER, C. J et al. Abundance patterns in early-type galaxies: is there a "knee" in the [Fe/H] vs. ['alfa'/Fe] relation?. Astronomy & Astrophysics, v. 582, p. A46/1-A46/20, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525924. Acesso em: 03 out. 2024.
APA
Walcher, C. J., Coelho, P. R. T., Gallazzi, A., Bruzual, G., Charlot, S., & Chiappini, C. (2015). Abundance patterns in early-type galaxies: is there a "knee" in the [Fe/H] vs. ['alfa'/Fe] relation? Astronomy & Astrophysics, 582, A46/1-A46/20. doi:10.1051/0004-6361/201525924
NLM
Walcher CJ, Coelho PRT, Gallazzi A, Bruzual G, Charlot S, Chiappini C. Abundance patterns in early-type galaxies: is there a "knee" in the [Fe/H] vs. ['alfa'/Fe] relation? [Internet]. Astronomy & Astrophysics. 2015 ; 582 A46/1-A46/20.[citado 2024 out. 03 ] Available from: https://doi.org/10.1051/0004-6361/201525924
Vancouver
Walcher CJ, Coelho PRT, Gallazzi A, Bruzual G, Charlot S, Chiappini C. Abundance patterns in early-type galaxies: is there a "knee" in the [Fe/H] vs. ['alfa'/Fe] relation? [Internet]. Astronomy & Astrophysics. 2015 ; 582 A46/1-A46/20.[citado 2024 out. 03 ] Available from: https://doi.org/10.1051/0004-6361/201525924
Trabalho de evento-resumo
The fossil record of the stellar populations at redshifts above 1.5 (2015)
Walcher, C. Jakob; Coelho, Paula Rodrigues Teixeira; Gallazzi, Anna; Charlot, Stéphane; Bruzual, Gustavo
Source: Meeting Abstracts. Conference titles: IAU General Assembly. Unidade: IAG
Assunto: POPULAÇÕES ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
WALCHER, C. Jakob et al. The fossil record of the stellar populations at redshifts above 1.5. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 03 out. 2024.
APA
Walcher, C. J., Coelho, P. R. T., Gallazzi, A., Charlot, S., & Bruzual, G. (2015). The fossil record of the stellar populations at redshifts above 1.5. In Meeting Abstracts. Paris: International Astronomical Union.
NLM
Walcher CJ, Coelho PRT, Gallazzi A, Charlot S, Bruzual G. The fossil record of the stellar populations at redshifts above 1.5. Meeting Abstracts. 2015 ;[citado 2024 out. 03 ]
Vancouver
Walcher CJ, Coelho PRT, Gallazzi A, Charlot S, Bruzual G. The fossil record of the stellar populations at redshifts above 1.5. Meeting Abstracts. 2015 ;[citado 2024 out. 03 ]

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