ReP USP - Resultado da busca

Artigo de periodico
r-Process abundances in metal-poor Galactic halo stars (2014)
Siqueira Mello, C; Barbuy, Beatriz Leonor Silveira; Spite, M; Spite, F; Caffau, E; Hill, V; Wanajo, S; François, P; Bonifacio, P; Cayrel, R
Source: Memorie della Società Astronomica Italiana. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA)
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SIQUEIRA MELLO, C et al. r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana, v. 85, p. 232-235, 2014Tradução . . Acesso em: 14 maio 2024.
APA
Siqueira Mello, C., Barbuy, B. L. S., Spite, M., Spite, F., Caffau, E., Hill, V., et al. (2014). r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana, 85, 232-235.
NLM
Siqueira Mello C, Barbuy BLS, Spite M, Spite F, Caffau E, Hill V, Wanajo S, François P, Bonifacio P, Cayrel R. r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana. 2014 ; 85 232-235.[citado 2024 maio 14 ]
Vancouver
Siqueira Mello C, Barbuy BLS, Spite M, Spite F, Caffau E, Hill V, Wanajo S, François P, Bonifacio P, Cayrel R. r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana. 2014 ; 85 232-235.[citado 2024 maio 14 ]
Artigo de periodico
UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3 (2014)
Keller, Graziela R; Bianchi, Luciana; Maciel, Walter Junqueira
Source: Monthly Notices Royal Astronomical Society. Unidade: IAG
Subjects: ESTRELAS, ATMOSFERAS ESTELARES, PERDA DE MASSA, VENTO
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KELLER, Graziela R e BIANCHI, Luciana e MACIEL, Walter Junqueira. UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3. Monthly Notices Royal Astronomical Society, v. 442, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnras/stu878. Acesso em: 14 maio 2024.
APA
Keller, G. R., Bianchi, L., & Maciel, W. J. (2014). UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3. Monthly Notices Royal Astronomical Society, 442. doi:10.1093/mnras/stu878
NLM
Keller GR, Bianchi L, Maciel WJ. UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3 [Internet]. Monthly Notices Royal Astronomical Society. 2014 ; 442[citado 2024 maio 14 ] Available from: https://doi.org/10.1093/mnras/stu878
Vancouver
Keller GR, Bianchi L, Maciel WJ. UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3 [Internet]. Monthly Notices Royal Astronomical Society. 2014 ; 442[citado 2024 maio 14 ] Available from: https://doi.org/10.1093/mnras/stu878
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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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.1051/0004-6361/201629941
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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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: 14 maio 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 maio 14 ] 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 maio 14 ] Available from: https://doi.org/10.1093/mnras/stz3609
Artigo de periodico
The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances (2008)
Zoccali, M; Hill, V; Lecureur, A; Barbuy, Beatriz Leonor Silveira; Renzini, A; Minniti, D; Gómez, A; Ortolani, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ZOCCALI, M et al. The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics, v. 486, p. 177-189, 2008Tradução . . Acesso em: 14 maio 2024.
APA
Zoccali, M., Hill, V., Lecureur, A., Barbuy, B. L. S., Renzini, A., Minniti, D., et al. (2008). The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics, 486, 177-189.
NLM
Zoccali M, Hill V, Lecureur A, Barbuy BLS, Renzini A, Minniti D, Gómez A, Ortolani S. The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics. 2008 ; 486 177-189.[citado 2024 maio 14 ]
Vancouver
Zoccali M, Hill V, Lecureur A, Barbuy BLS, Renzini A, Minniti D, Gómez A, Ortolani S. The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics. 2008 ; 486 177-189.[citado 2024 maio 14 ]
Artigo de periodico
The future of the Sun: an evolved solar twin revealed by CoRoT (2013)
Nascimento Júnior, J.-D. do; Takeda, Y; Moreno, Jorge Luis Meléndez; Costa, J. S. da; Mello, G. F. Porto de; Castro, M
Source: The Astrophysical Journal Letters. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS, SOL
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NASCIMENTO JÚNIOR, J.-D. do et al. The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, v. 771, p. L31/1-L31/5, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/771/2/L31. Acesso em: 14 maio 2024.
APA
Nascimento Júnior, J. -D. do, Takeda, Y., Moreno, J. L. M., Costa, J. S. da, Mello, G. F. P. de, & Castro, M. (2013). The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, 771, L31/1-L31/5. doi:10.1088/2041-8205/771/2/L31
NLM
Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 maio 14 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
Vancouver
Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 maio 14 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
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
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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.1093/mnras/stw1829
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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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.1093/mnrasl/slz153
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
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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.1093/mnras/stw2045
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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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
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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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
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
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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.1093/mnras/stw247
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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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
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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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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.1093/mnras/stz754
Artigo de periodico
Spectroscopic validation of low-metallicity stars from RAVE (2018)
Placco, Vinicius M; Beers, Johanna; Santucci, Rafael M; Chanamé, Julio; Rossi, Silvia Cristina Fernandes
Source: Astronomical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESPECTROSCOPIA
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ABNT
PLACCO, Vinicius M et al. Spectroscopic validation of low-metallicity stars from RAVE. Astronomical Journal, v. 155, n. 6, p. 256, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-3881/aac20c. Acesso em: 14 maio 2024.
APA
Placco, V. M., Beers, J., Santucci, R. M., Chanamé, J., & Rossi, S. C. F. (2018). Spectroscopic validation of low-metallicity stars from RAVE. Astronomical Journal, 155( 6), 256. doi:10.3847/1538-3881/aac20c
NLM
Placco VM, Beers J, Santucci RM, Chanamé J, Rossi SCF. Spectroscopic validation of low-metallicity stars from RAVE [Internet]. Astronomical Journal. 2018 ; 155( 6): 256.[citado 2024 maio 14 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
Vancouver
Placco VM, Beers J, Santucci RM, Chanamé J, Rossi SCF. Spectroscopic validation of low-metallicity stars from RAVE [Internet]. Astronomical Journal. 2018 ; 155( 6): 256.[citado 2024 maio 14 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
Artigo de periodico
Reddenings of Cepheids (2012)
Andrievsky, S. M; Luck, R. E; Kovtyukh, V. V; Lepine, Jacques Raymond Daniel
Source: Publications of the Astronomical Society of the Pacific. Unidade: IAG
Subjects: ESTRELAS, ATMOSFERAS ESTELARES, FOTOMETRIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ANDRIEVSKY, S. M et al. Reddenings of Cepheids. Publications of the Astronomical Society of the Pacific, v. 124, p. 934-938, 2012Tradução . . Disponível em: https://doi.org/10.1086/668085. Acesso em: 14 maio 2024.
APA
Andrievsky, S. M., Luck, R. E., Kovtyukh, V. V., & Lepine, J. R. D. (2012). Reddenings of Cepheids. Publications of the Astronomical Society of the Pacific, 124, 934-938. doi:10.1086/668085
NLM
Andrievsky SM, Luck RE, Kovtyukh VV, Lepine JRD. Reddenings of Cepheids [Internet]. Publications of the Astronomical Society of the Pacific. 2012 ; 124 934-938.[citado 2024 maio 14 ] Available from: https://doi.org/10.1086/668085
Vancouver
Andrievsky SM, Luck RE, Kovtyukh VV, Lepine JRD. Reddenings of Cepheids [Internet]. Publications of the Astronomical Society of the Pacific. 2012 ; 124 934-938.[citado 2024 maio 14 ] Available from: https://doi.org/10.1086/668085
Artigo de periodico
Oxygen, sodium, magnesium, and aluminium as tracers of the galactic bulge formation (2007)
Lecureur, A; Hill, V; Zoccali, M; Barbuy, Beatriz Leonor Silveira; Gómez, A; Minniti, D; Ortolani, S; Renzini, A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LECUREUR, A et al. Oxygen, sodium, magnesium, and aluminium as tracers of the galactic bulge formation. Astronomy & Astrophysics, v. 465, n. 3, p. 799-814, 2007Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20066036. Acesso em: 14 maio 2024.
APA
Lecureur, A., Hill, V., Zoccali, M., Barbuy, B. L. S., Gómez, A., Minniti, D., et al. (2007). Oxygen, sodium, magnesium, and aluminium as tracers of the galactic bulge formation. Astronomy & Astrophysics, 465( 3), 799-814. doi:10.1051/0004-6361:20066036
NLM
Lecureur A, Hill V, Zoccali M, Barbuy BLS, Gómez A, Minniti D, Ortolani S, Renzini A. Oxygen, sodium, magnesium, and aluminium as tracers of the galactic bulge formation [Internet]. Astronomy & Astrophysics. 2007 ;465( 3): 799-814.[citado 2024 maio 14 ] Available from: https://doi.org/10.1051/0004-6361:20066036
Vancouver
Lecureur A, Hill V, Zoccali M, Barbuy BLS, Gómez A, Minniti D, Ortolani S, Renzini A. Oxygen, sodium, magnesium, and aluminium as tracers of the galactic bulge formation [Internet]. Astronomy & Astrophysics. 2007 ;465( 3): 799-814.[citado 2024 maio 14 ] Available from: https://doi.org/10.1051/0004-6361:20066036
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 14 maio 2024.
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 2024 maio 14 ] 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 2024 maio 14 ] Available from: https://doi.org/10.3847/1538-4365/ab7660
Artigo de periodico
On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle (2009)
Groh, J.H; Hiller, J. D; Damineli Neto, Augusto; Withelock, P. A; Marang, F; Rossi, C
Source: The Astrophysical Journal. 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
GROH, J.H et al. On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal, v. 698, p. 1698-1720, 2009Tradução . . Acesso em: 14 maio 2024.
APA
Groh, J. H., Hiller, J. D., Damineli Neto, A., Withelock, P. A., Marang, F., & Rossi, C. (2009). On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal, 698, 1698-1720.
NLM
Groh JH, Hiller JD, Damineli Neto A, Withelock PA, Marang F, Rossi C. On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal. 2009 ; 698 1698-1720.[citado 2024 maio 14 ]
Vancouver
Groh JH, Hiller JD, Damineli Neto A, Withelock PA, Marang F, Rossi C. On the nature of the prototype luminous blue variable AG Carinae: I. Fundamental parameters during visual minimum phases and changes in bolometric luminosity during the S-Dor cycle. The Astrophysical Journal. 2009 ; 698 1698-1720.[citado 2024 maio 14 ]
Artigo de periodico
On the nature of the prototype luminous blue variable A G Carinae: II. Witnessing a massive star evolving close to the Eddington and bistability limits (2011)
Groh, J. H; Hillier, D. J; Damineli Neto, Augusto
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ATMOSFERAS ESTELARES, ESTRELAS VARIÁVEIS, PERDA DE MASSA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GROH, J. H e HILLIER, D. J e DAMINELI NETO, Augusto. On the nature of the prototype luminous blue variable A G Carinae: II. Witnessing a massive star evolving close to the Eddington and bistability limits. The Astrophysical Journal, v. 737, p. 46/1-46/13, 2011Tradução . . Acesso em: 14 maio 2024.
APA
Groh, J. H., Hillier, D. J., & Damineli Neto, A. (2011). On the nature of the prototype luminous blue variable A G Carinae: II. Witnessing a massive star evolving close to the Eddington and bistability limits. The Astrophysical Journal, 737, 46/1-46/13.
NLM
Groh JH, Hillier DJ, Damineli Neto A. On the nature of the prototype luminous blue variable A G Carinae: II. Witnessing a massive star evolving close to the Eddington and bistability limits. The Astrophysical Journal. 2011 ; 737 46/1-46/13.[citado 2024 maio 14 ]
Vancouver
Groh JH, Hillier DJ, Damineli Neto A. On the nature of the prototype luminous blue variable A G Carinae: II. Witnessing a massive star evolving close to the Eddington and bistability limits. The Astrophysical Journal. 2011 ; 737 46/1-46/13.[citado 2024 maio 14 ]

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