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Tese (Doutorado)
Análise crono-químiodinâmica de aglomerados globulares: procurando por fósseis da formação da barra/bojo galático (2024)
Souza, Stefano Oliveira; Barbuy, Beatriz (Orientador)
Unidade: IAG
Subjects: AGLOMERADOS (GALÁXIA), ATMOSFERAS ESTELARES
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ABNT
SOUZA, Stefano Oliveira. Análise crono-químiodinâmica de aglomerados globulares: procurando por fósseis da formação da barra/bojo galático. 2024. Tese (Doutorado) – Universidade de São Paulo, São Paulo, 2024. . Acesso em: 24 abr. 2026.
APA
Souza, S. O. (2024). Análise crono-químiodinâmica de aglomerados globulares: procurando por fósseis da formação da barra/bojo galático (Tese (Doutorado). Universidade de São Paulo, São Paulo.
NLM
Souza SO. Análise crono-químiodinâmica de aglomerados globulares: procurando por fósseis da formação da barra/bojo galático. 2024 ;[citado 2026 abr. 24 ]
Vancouver
Souza SO. Análise crono-químiodinâmica de aglomerados globulares: procurando por fósseis da formação da barra/bojo galático. 2024 ;[citado 2026 abr. 24 ]
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
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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: 24 abr. 2026.
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 2026 abr. 24 ] 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 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stab3789
Artigo de periodico
Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid (2022)
Razera, R ; Barbuy, Beatriz Leonor Silveira ; Moura, T. C ; Ernandes, H ; Friaça, Amâncio César Santos
Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IF
Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS
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ABNT
RAZERA, R et al. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, v. 517, p. 4590-4606, 2022Tradução . . Disponível em: https://academic.oup.com/mnras/article/517/3/4590/6653110. Acesso em: 24 abr. 2026.
APA
Razera, R., Barbuy, B. L. S., Moura, T. C., Ernandes, H., & Friaça, A. C. S. (2022). Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, 517, 4590-4606. doi:10.1093/mnras/stac2136
NLM
Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2026 abr. 24 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
Vancouver
Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2026 abr. 24 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
Artigo de periodico
One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field (2020)
Barbosa, Carlos Eduardo ; Oliveira, Claudia Lucia Mendes de ; Molino, Alberto ; Costa-Duarte, M. V; Coelho, Paula Rodrigues Teixeira ; Cortesi, Arianna ; Herpich, Fábio R ; Hernandez-Jimenez, J. A; Santos-Silva, T; Pereira, Eduardo S ; Werle, Ariel ; Overzier, Roderik ; Ribeiro, T
Source: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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ABNT
BARBOSA, Carlos Eduardo et al. One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v. 231, n. 1, p. 1, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/ab7660. Acesso em: 24 abr. 2026.
APA
Barbosa, C. E., Oliveira, C. L. M. de, Molino, A., Costa-Duarte, M. V., Coelho, P. R. T., Cortesi, A., et al. (2020). One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 231( 1), 1. doi:10.3847/1538-4365/ab7660
NLM
Barbosa CE, Oliveira CLM de, Molino A, Costa-Duarte MV, Coelho PRT, Cortesi A, Herpich FR, Hernandez-Jimenez JA, Santos-Silva T, Pereira ES, Werle A, Overzier R, Ribeiro T. One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2020 ;231( 1): 1.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/ab7660
Vancouver
Barbosa CE, Oliveira CLM de, Molino A, Costa-Duarte MV, Coelho PRT, Cortesi A, Herpich FR, Hernandez-Jimenez JA, Santos-Silva T, Pereira ES, Werle A, Overzier R, Ribeiro T. One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2020 ;231( 1): 1.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/ab7660
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
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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: 24 abr. 2026.
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 2026 abr. 24 ] 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 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stz3609
Artigo de periodico
The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo* (2020)
Holmbeck, Erika M.
Source: Astrophysical Journal Supplement Series. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
HOLMBECK, Erika M. The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo*. Astrophysical Journal Supplement Series, v. 249, p. 30, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/ab9c19. Acesso em: 24 abr. 2026.
APA
Holmbeck, E. M. (2020). The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo*. Astrophysical Journal Supplement Series, 249, 30. doi:10.3847/1538-4365/ab9c19
NLM
Holmbeck EM. The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo* [Internet]. Astrophysical Journal Supplement Series. 2020 ; 249 30.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
Vancouver
Holmbeck EM. The R-Process Alliance:: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo* [Internet]. Astrophysical Journal Supplement Series. 2020 ; 249 30.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
Artigo de periodico
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters (2020)
Oliveira, R. A. P. ; Souza, S. O ; keber, L. O ; Barbuy, Beatriz Leonor Silveira
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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ABNT
OLIVEIRA, R. A. P. et al. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6f76. Acesso em: 24 abr. 2026.
APA
Oliveira, R. A. P., Souza, S. O., keber, L. O., & Barbuy, B. L. S. (2020). The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab6f76
NLM
Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
Vancouver
Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
Artigo de periodico
Integrated Spectra of Milky Way Globular Clusters (2019)
Moura, T. C; Trevisan, M; Barbuy, Beatriz Leonor Silveira; Rossi, Silvia Cristina Fernandes
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES
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ABNT
MOURA, T. C et al. Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab3eb6. Acesso em: 24 abr. 2026.
APA
Moura, T. C., Trevisan, M., Barbuy, B. L. S., & Rossi, S. C. F. (2019). Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab3eb6
NLM
Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
Vancouver
Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
Artigo de periodico
J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX (2019)
Whitten, D. D; Coelho, Paula Rodrigues Teixeira; Costa-Duarte, M. V; Oliveira, Claudia Lucia Mendes de; Rossi, Silvia Cristina Fernandes; Sodré Júnior, Laerte; Hernandez-Jimenez, P
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: FOTOMETRIA, ATMOSFERAS ESTELARES
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ABNT
WHITTEN, D. D et al. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX. Astronomy & Astrophysics, v. 622, p. A182, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833368. Acesso em: 24 abr. 2026.
APA
Whitten, D. D., Coelho, P. R. T., Costa-Duarte, M. V., Oliveira, C. L. M. de, Rossi, S. C. F., Sodré Júnior, L., & Hernandez-Jimenez, P. (2019). J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX. Astronomy & Astrophysics, 622, A182. doi:10.1051/0004-6361/201833368
NLM
Whitten DD, Coelho PRT, Costa-Duarte MV, Oliveira CLM de, Rossi SCF, Sodré Júnior L, Hernandez-Jimenez P. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX [Internet]. Astronomy & Astrophysics. 2019 ; 622 A182.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201833368
Vancouver
Whitten DD, Coelho PRT, Costa-Duarte MV, Oliveira CLM de, Rossi SCF, Sodré Júnior L, Hernandez-Jimenez P. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX [Internet]. Astronomy & Astrophysics. 2019 ; 622 A182.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201833368
Artigo de periodico
Stellar spectral models compared with empirical data (2019)
Knowles, Adam T; Sansom, A. E; Coelho, Paula Rodrigues Teixeira ; Prieto, C. Allende; Conroy, C; Vazdekis, A
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESPECTROSCOPIA
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ABNT
KNOWLES, Adam T et al. Stellar spectral models compared with empirical data. Monthly Notices of the Royal Astronomical Society, v. 486, n. 2, p. 1814-1832, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz754. Acesso em: 24 abr. 2026.
APA
Knowles, A. T., Sansom, A. E., Coelho, P. R. T., Prieto, C. A., Conroy, C., & Vazdekis, A. (2019). Stellar spectral models compared with empirical data. Monthly Notices of the Royal Astronomical Society, 486( 2), 1814-1832. doi:10.1093/mnras/stz754
NLM
Knowles AT, Sansom AE, Coelho PRT, Prieto CA, Conroy C, Vazdekis A. Stellar spectral models compared with empirical data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 2): 1814-1832.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stz754
Vancouver
Knowles AT, Sansom AE, Coelho PRT, Prieto CA, Conroy C, Vazdekis A. Stellar spectral models compared with empirical data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 2): 1814-1832.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stz754
Artigo de periodico
The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey (2019)
Placco, Vinicius M; Santucci, Rafael M; Rossi, Silvia Cristina Fernandes
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
PLACCO, Vinicius M e SANTUCCI, Rafael M e ROSSI, Silvia Cristina Fernandes. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, v. 870, n. 2, p. 122-1/122-11, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf3b9. Acesso em: 24 abr. 2026.
APA
Placco, V. M., Santucci, R. M., & Rossi, S. C. F. (2019). The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, 870( 2), 122-1/122-11. doi:10.3847/1538-4357/aaf3b9
NLM
Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
Vancouver
Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
Artigo de periodico
The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 (2019)
Galarza, Jhon Yana; Meléndez, Jorge; Lorenzo-Oliveira, Diego; Reggiani, Henrique; Carlos, Marília; Ponte, Geisa
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESPECTROMETRIA, ATMOSFERAS ESTELARES
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ABNT
GALARZA, Jhon Yana et al. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, v. 490, p. L86-L90, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slz153. Acesso em: 24 abr. 2026.
APA
Galarza, J. Y., Meléndez, J., Lorenzo-Oliveira, D., Reggiani, H., Carlos, M., & Ponte, G. (2019). The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, 490, L86-L90. doi:10.1093/mnrasl/slz153
NLM
Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnrasl/slz153
Vancouver
Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnrasl/slz153
Artigo de periodico
High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725 (2017)
Santrich, Orlando J. Katime; Rossi, Silvia Cristina Fernandes
Source: Canadian Journal of Physics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, EVOLUÇÃO ESTELAR
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ABNT
SANTRICH, Orlando J. Katime e ROSSI, Silvia Cristina Fernandes. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. Canadian Journal of Physics, v. 95, n. 9, p. 862-868, 2017Tradução . . Disponível em: https://doi.org/10.1139/cjp-2016-0912. Acesso em: 24 abr. 2026.
APA
Santrich, O. J. K., & Rossi, S. C. F. (2017). High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. Canadian Journal of Physics, 95( 9), 862-868. doi:10.1139/cjp-2016-0912
NLM
Santrich OJK, Rossi SCF. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725 [Internet]. Canadian Journal of Physics. 2017 ; 95( 9): 862-868.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1139/cjp-2016-0912
Vancouver
Santrich OJK, Rossi SCF. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725 [Internet]. Canadian Journal of Physics. 2017 ; 95( 9): 862-868.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1139/cjp-2016-0912
Artigo de periodico
Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* (2017)
Friaça, Amâncio César Santos; Barbuy, Beatriz Leonor Silveira
Source: Astronomy and Astrophysysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, GALÁXIAS
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ABNT
FRIAÇA, Amâncio César Santos e BARBUY, Beatriz Leonor Silveira. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements*. Astronomy and Astrophysysics, v. 598, p. A121, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629941. Acesso em: 24 abr. 2026.
APA
Friaça, A. C. S., & Barbuy, B. L. S. (2017). Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements*. Astronomy and Astrophysysics, 598, A121. doi:10.1051/0004-6361/201629941
NLM
Friaça ACS, Barbuy BLS. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* [Internet]. Astronomy and Astrophysysics. 2017 ;598 A121.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201629941
Vancouver
Friaça ACS, Barbuy BLS. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* [Internet]. Astronomy and Astrophysysics. 2017 ;598 A121.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201629941
Artigo de periodico
A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis (2017)
Levenhagem, Ronaldo Savarino; Diaz, Marcos Perez; Coelho, Paula Rodrigues Teixeira; Hubeny, Ivan
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: 24 abr. 2026.
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 2026 abr. 24 ] 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 2026 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/aa7681
Artigo de periodico
The chemical compositions of solar twins in the open cluster M67 (2016)
Asplund, F; Asplund, M; Yong, D; Moreno, Jorge Luiz Meléndez; Ramírez, I; Karakas, A. I; Carlos, M; Marino, A. F
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ASPLUND, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, v. 463, p. 696-704, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 24 abr. 2026.
APA
Asplund, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 463, 696-704. doi:10.1093/mnras/stw2045
NLM
Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stw2045
Vancouver
Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stw2045
Artigo de periodico
Looking for imprints of the first stellar generations in metal-poor bulge field stars (2016)
Siqueira-Mello, C; Chiappini, C; Barbuy, Beatriz Leonor Silveira; Cantelli, E
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: CENTRO GALÁCTICO, 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. Looking for imprints of the first stellar generations in metal-poor bulge field stars. Astronomy & Astrophysics, v. 593, p. A79/1-A79/16, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628104. Acesso em: 24 abr. 2026.
APA
Siqueira-Mello, C., Chiappini, C., Barbuy, B. L. S., & Cantelli, E. (2016). Looking for imprints of the first stellar generations in metal-poor bulge field stars. Astronomy & Astrophysics, 593, A79/1-A79/16. doi:10.1051/0004-6361/201628104
NLM
Siqueira-Mello C, Chiappini C, Barbuy BLS, Cantelli E. Looking for imprints of the first stellar generations in metal-poor bulge field stars [Internet]. Astronomy & Astrophysics. 2016 ; 593 A79/1-A79/16.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201628104
Vancouver
Siqueira-Mello C, Chiappini C, Barbuy BLS, Cantelli E. Looking for imprints of the first stellar generations in metal-poor bulge field stars [Internet]. Astronomy & Astrophysics. 2016 ; 593 A79/1-A79/16.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201628104
Artigo de periodico
The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle (2016)
Gull, Theodore R; Madura, Thomas I; Teodoro, Mairan; Clementel, Nicola; Corcoran, Michael; Damineli Neto, Augusto; Groh, Jose H; Hamaguchi, Kenji; Hillier, D. John; Moffat, Anthony F. J; Richardson, Noel D; Weigelt, Gerd; Lindler, Don; Feggans, Keith
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ESTRELAS, PERDA DE MASSA, ESTRELAS VARIÁVEIS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GULL, Theodore R et al. The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle. Monthly Notices of the Royal Astronomical Society, v. 462, p. 3196-3220, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw1829. Acesso em: 24 abr. 2026.
APA
Gull, T. R., Madura, T. I., Teodoro, M., Clementel, N., Corcoran, M., Damineli Neto, A., et al. (2016). The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle. Monthly Notices of the Royal Astronomical Society, 462, 3196-3220. doi:10.1093/mnras/stw1829
NLM
Gull TR, Madura TI, Teodoro M, Clementel N, Corcoran M, Damineli Neto A, Groh JH, Hamaguchi K, Hillier DJ, Moffat AFJ, Richardson ND, Weigelt G, Lindler D, Feggans K. The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 462 3196-3220.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stw1829
Vancouver
Gull TR, Madura TI, Teodoro M, Clementel N, Corcoran M, Damineli Neto A, Groh JH, Hamaguchi K, Hillier DJ, Moffat AFJ, Richardson ND, Weigelt G, Lindler D, Feggans K. The fossil wind structures of Eta Carinae: changes across one 5.54-yr cycle [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 462 3196-3220.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stw1829
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: 24 abr. 2026.
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 2026 abr. 24 ] 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 2026 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201525709
Artigo de periodico
The Hyades open cluster is chemically inhomogeneous (2016)
Liu, F; Yong, D; Asplund, M; Ramírez, I; Moreno, Jorge Luiz Meléndez
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LIU, F et al. The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, v. 457, p. 3934-3948, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw247. Acesso em: 24 abr. 2026.
APA
Liu, F., Yong, D., Asplund, M., Ramírez, I., & Moreno, J. L. M. (2016). The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, 457, 3934-3948. doi:10.1093/mnras/stw247
NLM
Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stw247
Vancouver
Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2026 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stw247

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