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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
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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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] 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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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz3609
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnrasl/slz153
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz754
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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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: 18 nov. 2024.
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 2024 nov. 18 ] 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 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201833368
Artigo de periodico
Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres (2018)
Spina, Lorenzo; Moreno, Jorge Luis Meléndez; Casey, Andrew R; Karakas, Amanda I; Tucci-Maia, Marcelo
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
SPINA, Lorenzo et al. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, v. 863, n. 2, p. 179-1/179-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 18 nov. 2024.
APA
Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
NLM
Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/aad190
Vancouver
Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/aad190
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
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: 18 nov. 2024.
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 2024 nov. 18 ] 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 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/aa7681
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: 18 nov. 2024.
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 2024 nov. 18 ] 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 2024 nov. 18 ] Available from: https://doi.org/10.1139/cjp-2016-0912
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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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stw247
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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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stw1829
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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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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stw2045
Trabalho de evento
Circumstellar polarimetry (2015)
Magalhães, Antonio Mário; Carciofi, Alex Cavaliéri; Seriacopi, D. B
Source: Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. Conference titles: IAU Symposium. Unidade: IAG
Subjects: POLARIZAÇÃO (ASTRONOMIA), TRANSFERÊNCIA RADIATIVA, ATMOSFERAS ESTELARES
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ABNT
MAGALHÃES, Antonio Mário e CARCIOFI, Alex Cavaliéri e SERIACOPI, D. B. Circumstellar polarimetry. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921315004871. Acesso em: 18 nov. 2024.
APA
Magalhães, A. M., Carciofi, A. C., & Seriacopi, D. B. (2015). Circumstellar polarimetry. In Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. Paris: International Astronomical Union. doi:10.1017/S1743921315004871
NLM
Magalhães AM, Carciofi AC, Seriacopi DB. Circumstellar polarimetry [Internet]. Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. 2015 ;[citado 2024 nov. 18 ] Available from: https://doi.org/10.1017/S1743921315004871
Vancouver
Magalhães AM, Carciofi AC, Seriacopi DB. Circumstellar polarimetry [Internet]. Polarimetry:from the Sun to Stars and Stellar Environments: Proceedings of IAU Symposium, 305. 2015 ;[citado 2024 nov. 18 ] Available from: https://doi.org/10.1017/S1743921315004871
Artigo de periodico
Discovery of the massive overcontact binary VFTS352: evidence for enhanced internal mixing (2015)
Almeida, L. A; Sana, H; de Mink, S. E; Tramper, F; Soszynski, I; Langer, N; Barbá, R. H; Cantiello, M; Damineli Neto, Augusto; Koter, A. de; García, M; Gräfener, G; Herrero, A; Horvath, I; Maíz-Apellániz, J; Norman, C; Ramírez-Agudelo, O. H; Vink, J. S
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, ATMOSFERAS ESTELARES
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ABNT
ALMEIDA, L. A et al. Discovery of the massive overcontact binary VFTS352: evidence for enhanced internal mixing. The Astrophysical Journal, v. 812, p. 102/1-102/9, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/812/2/102. Acesso em: 18 nov. 2024.
APA
Almeida, L. A., Sana, H., de Mink, S. E., Tramper, F., Soszynski, I., Langer, N., et al. (2015). Discovery of the massive overcontact binary VFTS352: evidence for enhanced internal mixing. The Astrophysical Journal, 812, 102/1-102/9. doi:10.1088/0004-637X/812/2/102
NLM
Almeida LA, Sana H, de Mink SE, Tramper F, Soszynski I, Langer N, Barbá RH, Cantiello M, Damineli Neto A, Koter A de, García M, Gräfener G, Herrero A, Horvath I, Maíz-Apellániz J, Norman C, Ramírez-Agudelo OH, Vink JS. Discovery of the massive overcontact binary VFTS352: evidence for enhanced internal mixing [Internet]. The Astrophysical Journal. 2015 ; 812 102/1-102/9.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1088/0004-637X/812/2/102
Vancouver
Almeida LA, Sana H, de Mink SE, Tramper F, Soszynski I, Langer N, Barbá RH, Cantiello M, Damineli Neto A, Koter A de, García M, Gräfener G, Herrero A, Horvath I, Maíz-Apellániz J, Norman C, Ramírez-Agudelo OH, Vink JS. Discovery of the massive overcontact binary VFTS352: evidence for enhanced internal mixing [Internet]. The Astrophysical Journal. 2015 ; 812 102/1-102/9.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1088/0004-637X/812/2/102
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stu878
Artigo de periodico
Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5 (2014)
Placco, Vinicius M; Frebel, Anna; Beers, Timothy C; Beers, Timothy C; Christlieb, Norbert; Lee, Young Sun; Kennedy, Catherine R; Rossi, Silvia Cristina Fernandes; Santucci, Rafael Miloni
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, ESPECTROSCOPIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
PLACCO, Vinicius M et al. Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5. The Astrophysical Journal, v. 781, n. 40, p. 1-14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/781/1/40. Acesso em: 18 nov. 2024.
APA
Placco, V. M., Frebel, A., Beers, T. C., Beers, T. C., Christlieb, N., Lee, Y. S., et al. (2014). Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5. The Astrophysical Journal, 781( 40), 1-14. doi:10.1088/0004-637X/781/1/40
NLM
Placco VM, Frebel A, Beers TC, Beers TC, Christlieb N, Lee YS, Kennedy CR, Rossi SCF, Santucci RM. Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H]<= -3,5 [Internet]. The Astrophysical Journal. 2014 ; 781( 40): 1-14.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1088/0004-637X/781/1/40
Vancouver
Placco VM, Frebel A, Beers TC, Beers TC, Christlieb N, Lee YS, Kennedy CR, Rossi SCF, Santucci RM. Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H]<= -3,5 [Internet]. The Astrophysical Journal. 2014 ; 781( 40): 1-14.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1088/0004-637X/781/1/40
Artigo de periodico
A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation (2014)
Liu, F; Asplund, M; Ramírez, I; Yong, D; Moreno, Jorge Luiz Meléndez
Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, FORMAÇÃO DO SISTEMA SOLAR, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS BINÁRIAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LIU, F et al. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, v. 442, p. L51-L55, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slu055. Acesso em: 18 nov. 2024.
APA
Liu, F., Asplund, M., Ramírez, I., Yong, D., & Moreno, J. L. M. (2014). A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, 442, L51-L55. doi:10.1093/mnrasl/slu055
NLM
Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1093/mnrasl/slu055
Vancouver
Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1093/mnrasl/slu055
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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ABNT
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: 18 nov. 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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31

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