ReP USP - Resultado da busca

Artigo de periodico
Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy (2022)
Ernandes, H ; Barbuy, Beatriz Leonor Silveira ; Friaça, Amâncio César Santos; Hill, V; Spite, M; Spite, F; Castilho, B. V; Evans, C. J
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ERNANDES, H et al. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, v. 510, p. 5362-5375, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3789. Acesso em: 20 out. 2024.
APA
Ernandes, H., Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Spite, M., Spite, F., et al. (2022). Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, 510, 5362-5375. doi:10.1093/mnras/stab3789
NLM
Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stab3789
Vancouver
Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 out. 20 ] Available from: https://doi.org/10.1093/mnras/stab3789
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: 20 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. 20 ] 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. 20 ] Available from: https://doi.org/10.1093/mnras/stz3609
Artigo de periodico
Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants (2016)
van der Swaelmen, M; Barbuy, Beatriz Leonor Silveira; Hill, V; Zoccali, M; Minniti, D; Ortolani, S; Gómez, A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, GALÁXIA (VIA LÁCTEA)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
VAN DER SWAELMEN, M et al. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, v. 586, p. A1/1-A1/11, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525709. Acesso em: 20 out. 2024.
APA
van der Swaelmen, M., Barbuy, B. L. S., Hill, V., Zoccali, M., Minniti, D., Ortolani, S., & Gómez, A. (2016). Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, 586, A1/1-A1/11. doi:10.1051/0004-6361/201525709
NLM
van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201525709
Vancouver
van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201525709
Artigo de periodico
High-resolution abundance analysis of HD 140283 (2015)
Siqueira Mello, C; Andrievsky, S. M; Barbuy, Beatriz Leonor Silveira; Spite, M; Spite, F; Korotin, S. A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ASTROFÍSICA ESTELAR, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SIQUEIRA MELLO, C et al. High-resolution abundance analysis of HD 140283. Astronomy & Astrophysics, v. 584, p. A86/1-A86/19, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526695. Acesso em: 20 out. 2024.
APA
Siqueira Mello, C., Andrievsky, S. M., Barbuy, B. L. S., Spite, M., Spite, F., & Korotin, S. A. (2015). High-resolution abundance analysis of HD 140283. Astronomy & Astrophysics, 584, A86/1-A86/19. doi:10.1051/0004-6361/201526695
NLM
Siqueira Mello C, Andrievsky SM, Barbuy BLS, Spite M, Spite F, Korotin SA. High-resolution abundance analysis of HD 140283 [Internet]. Astronomy & Astrophysics. 2015 ; 584 A86/1-A86/19.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201526695
Vancouver
Siqueira Mello C, Andrievsky SM, Barbuy BLS, Spite M, Spite F, Korotin SA. High-resolution abundance analysis of HD 140283 [Internet]. Astronomy & Astrophysics. 2015 ; 584 A86/1-A86/19.[citado 2024 out. 20 ] Available from: https://doi.org/10.1051/0004-6361/201526695

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