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Artigo de periodico
The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters (2018)
Chojnowski, S. Drew; Labadie-Bartz, Jonathan; Rivinius, Thomas; Gies, Douglas; Leister, Nelson Vani
Source: Astrophysical Journal. Unidade: IAG
Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR
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ABNT
CHOJNOWSKI, S. Drew et al. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, v. 865, n. 1, p. 76-1/76-16, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad964. Acesso em: 06 maio 2024.
APA
Chojnowski, S. D., Labadie-Bartz, J., Rivinius, T., Gies, D., & Leister, N. V. (2018). The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters. Astrophysical Journal, 865( 1), 76-1/76-16. doi:10.3847/1538-4357/aad964
NLM
Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 maio 06 ] Available from: https://doi.org/10.3847/1538-4357/aad964
Vancouver
Chojnowski SD, Labadie-Bartz J, Rivinius T, Gies D, Leister NV. The remarkable Be+sdOB Binary HD 55606. I. Orbital and stellar parameters [Internet]. Astrophysical Journal. 2018 ; 865( 1): 76-1/76-16.[citado 2024 maio 06 ] Available from: https://doi.org/10.3847/1538-4357/aad964
Artigo de periodico
The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios (2016)
Thygesen, A. O; Sbordone, L; Ludwig, H.-G; Ventura, P; Yong, D; Collet, R; Christlieb, N; Moreno, Jorge Luiz Meléndez; Zaggia, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA
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ABNT
THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 06 maio 2024.
APA
Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 588, A66. doi:10.1051/0004-6361/201526643
NLM
Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 maio 06 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
Vancouver
Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 maio 06 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
Artigo de periodico
The Li-age correlation: the sun is unusually Li deficient for its age (2019)
Carlos, Marilia; Moreno, Jorge Luiz Meléndez ; Spina, L; dos Santos, L. A; Bedell, M; Ramirez, I; Asplund, M; Bean, J. L; Yong, D; Yana Galarza, J; Alves-Brito, A
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ESPECTROSCOPIA, ABUNDANCIAS SOLARES
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ABNT
CARLOS, Marilia et al. The Li-age correlation: the sun is unusually Li deficient for its age. Monthly Notices of the Royal Astronomical Society, v. 485, p. 4052-4059, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 06 maio 2024.
APA
Carlos, M., Moreno, J. L. M., Spina, L., dos Santos, L. A., Bedell, M., Ramirez, I., et al. (2019). The Li-age correlation: the sun is unusually Li deficient for its age. Monthly Notices of the Royal Astronomical Society, 485, 4052-4059. doi:10.1093/mnras/slz681
NLM
Carlos M, Moreno JLM, Spina L, dos Santos LA, Bedell M, Ramirez I, Asplund M, Bean JL, Yong D, Yana Galarza J, Alves-Brito A. The Li-age correlation: the sun is unusually Li deficient for its age [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 485 4052-4059.[citado 2024 maio 06 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Vancouver
Carlos M, Moreno JLM, Spina L, dos Santos LA, Bedell M, Ramirez I, Asplund M, Bean JL, Yong D, Yana Galarza J, Alves-Brito A. The Li-age correlation: the sun is unusually Li deficient for its age [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 485 4052-4059.[citado 2024 maio 06 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
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: 06 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 06 ] 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 06 ] 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: 06 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 06 ] 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 06 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
Artigo de periodico
Spatial field reconstruction with INLA: application to IFU galaxy data (2019)
Gonzalez-Gaitan, S; Souza, R. S de; Krone-Martins, A; Cameron, E; Coelho, Paula Rodrigues Teixeira ; Galbany, L; Ishida, E. E. O
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: GALÁXIAS, ESPECTROSCOPIA, PROCESSAMENTO DE IMAGENS
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ABNT
GONZALEZ-GAITAN, S et al. Spatial field reconstruction with INLA: application to IFU galaxy data. Monthly Notices of the Royal Astronomical Society, v. 482, n. 3, p. 3880-3891, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty2881. Acesso em: 06 maio 2024.
APA
Gonzalez-Gaitan, S., Souza, R. S. de, Krone-Martins, A., Cameron, E., Coelho, P. R. T., Galbany, L., & Ishida, E. E. O. (2019). Spatial field reconstruction with INLA: application to IFU galaxy data. Monthly Notices of the Royal Astronomical Society, 482( 3), 3880-3891. doi:10.1093/mnras/sty2881
NLM
Gonzalez-Gaitan S, Souza RS de, Krone-Martins A, Cameron E, Coelho PRT, Galbany L, Ishida EEO. Spatial field reconstruction with INLA: application to IFU galaxy data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 3): 3880-3891.[citado 2024 maio 06 ] Available from: https://doi.org/10.1093/mnras/sty2881
Vancouver
Gonzalez-Gaitan S, Souza RS de, Krone-Martins A, Cameron E, Coelho PRT, Galbany L, Ishida EEO. Spatial field reconstruction with INLA: application to IFU galaxy data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 482( 3): 3880-3891.[citado 2024 maio 06 ] Available from: https://doi.org/10.1093/mnras/sty2881
Trabalho de evento-resumo
O-type binaries in 30 Dor: spectroscopic orbits, fundamental parameters, and distance to this region (2015)
Almeida, Leonardo Andrade; Sana, Hugues; Damineli Neto, Augusto
Source: Livro de resumos. Conference titles: Reunião Anual da Sociedade Astronômica Brasileira. Unidade: IAG
Subjects: ESTRELAS BINÁRIAS, ESPECTROSCOPIA
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ABNT
ALMEIDA, Leonardo Andrade e SANA, Hugues e DAMINELI NETO, Augusto. O-type binaries in 30 Dor: spectroscopic orbits, fundamental parameters, and distance to this region. 2015, Anais.. São Paulo: Sociedade Astronômica Brasileira, 2015. Disponível em: http://www.sab-astro.org.br/resources/Documents/ReunioesAnuais/2015/boletim-2015.pdf. Acesso em: 06 maio 2024.
APA
Almeida, L. A., Sana, H., & Damineli Neto, A. (2015). O-type binaries in 30 Dor: spectroscopic orbits, fundamental parameters, and distance to this region. In Livro de resumos. São Paulo: Sociedade Astronômica Brasileira. Recuperado de http://www.sab-astro.org.br/resources/Documents/ReunioesAnuais/2015/boletim-2015.pdf
NLM
Almeida LA, Sana H, Damineli Neto A. O-type binaries in 30 Dor: spectroscopic orbits, fundamental parameters, and distance to this region [Internet]. Livro de resumos. 2015 ;[citado 2024 maio 06 ] Available from: http://www.sab-astro.org.br/resources/Documents/ReunioesAnuais/2015/boletim-2015.pdf
Vancouver
Almeida LA, Sana H, Damineli Neto A. O-type binaries in 30 Dor: spectroscopic orbits, fundamental parameters, and distance to this region [Internet]. Livro de resumos. 2015 ;[citado 2024 maio 06 ] Available from: http://www.sab-astro.org.br/resources/Documents/ReunioesAnuais/2015/boletim-2015.pdf
Trabalho de evento
Low-mass eclipsing binaries in the WFCAM transit survey (2017)
Cruz, Patricia; Diaz, Marcos Perez; Barrado, David; Birkby, Jayne
Source: Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Conference titles: IAU SYMPOSIUM. Unidade: IAG
Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR
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ABNT
CRUZ, Patricia et al. Low-mass eclipsing binaries in the WFCAM transit survey. 2017, Anais.. Cambridge: Cambridge University Press, 2017. Disponível em: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003659. Acesso em: 06 maio 2024.
APA
Cruz, P., Diaz, M. P., Barrado, D., & Birkby, J. (2017). Low-mass eclipsing binaries in the WFCAM transit survey. In Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. Cambridge: Cambridge University Press. doi:10.1017/S1743921317003659
NLM
Cruz P, Diaz MP, Barrado D, Birkby J. Low-mass eclipsing binaries in the WFCAM transit survey [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 maio 06 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003659
Vancouver
Cruz P, Diaz MP, Barrado D, Birkby J. Low-mass eclipsing binaries in the WFCAM transit survey [Internet]. Living around active stars: proceedings of the 328th symposium of the IAU held in Maresias, Brazil October 17-21, 2016. 2017 ;[citado 2024 maio 06 ] Available from: https://doi-org.ez67.periodicos.capes.gov.br/10.1017/S1743921317003659
Trabalho de evento-resumo
High-coercivity, thermally stable and low unblocking temperature magnetic phase: implications for archeomagnetic studies (2013)
Hartmann, Gelvam ; Gallet, Yves; Trindade, Ricardo Ivan Ferreira da ; Ganevey, Agnès; Berquo, Thelma ; Neumann, Reiner; Le Goff, Maxime
Conference titles: AGU Meeting of the Americas 2013. Unidade: IAG
Subjects: GEOMAGNETISMO, PALEOMAGNETISMO, ESPECTROSCOPIA
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ABNT
HARTMANN, Gelvam et al. High-coercivity, thermally stable and low unblocking temperature magnetic phase: implications for archeomagnetic studies. 2013, Anais.. Washigton: American Geophysical Union, 2013. . Acesso em: 06 maio 2024.
APA
Hartmann, G., Gallet, Y., Trindade, R. I. F. da, Ganevey, A., Berquo, T., Neumann, R., & Le Goff, M. (2013). High-coercivity, thermally stable and low unblocking temperature magnetic phase: implications for archeomagnetic studies. In . Washigton: American Geophysical Union.
NLM
Hartmann G, Gallet Y, Trindade RIF da, Ganevey A, Berquo T, Neumann R, Le Goff M. High-coercivity, thermally stable and low unblocking temperature magnetic phase: implications for archeomagnetic studies. 2013 ;[citado 2024 maio 06 ]
Vancouver
Hartmann G, Gallet Y, Trindade RIF da, Ganevey A, Berquo T, Neumann R, Le Goff M. High-coercivity, thermally stable and low unblocking temperature magnetic phase: implications for archeomagnetic studies. 2013 ;[citado 2024 maio 06 ]
Artigo de periodico
Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis (2017)
Beers, Timothy C; Placco, Vinicius M; Carollo, Daniela; Rossi, Silvia Cristina Fernandes; Lee, Young Sun; Frebel, Anna; Norris, John E; Dietz, Sarah; Masseron, Thomas
Source: The Astrophysical Journal. Unidade: IAG
Subjects: CATÁLOGOS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS, CARBONO, ESPECTROSCOPIA
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ABNT
BEERS, Timothy C et al. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, v. 835, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 06 maio 2024.
APA
Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, 835, 81. doi:10.3847/1538-4357/835/1/81
NLM
Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 maio 06 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
Vancouver
Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 maio 06 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
Artigo de periodico
A Spectroscopic Orbit for the late-type Be star β CMi (2017)
Dulaney, Nicholas A; Richardson, Noel D; Gerhartz, Cody J; Carciofi, Alex Cavaliéri
Source: Astrophysical Journal. Unidade: IAG
Subjects: ESPECTROSCOPIA, ASTROFÍSICA ESTELAR
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ABNT
DULANEY, Nicholas A et al. A Spectroscopic Orbit for the late-type Be star β CMi. Astrophysical Journal, v. 836, n. 1, p. 112, 2017Tradução . . Disponível em: https://arxiv.org/abs/1701.05201. Acesso em: 06 maio 2024.
APA
Dulaney, N. A., Richardson, N. D., Gerhartz, C. J., & Carciofi, A. C. (2017). A Spectroscopic Orbit for the late-type Be star β CMi. Astrophysical Journal, 836( 1), 112. doi:10.3847/1538-4357/836/1/112
NLM
Dulaney NA, Richardson ND, Gerhartz CJ, Carciofi AC. A Spectroscopic Orbit for the late-type Be star β CMi [Internet]. Astrophysical Journal. 2017 ;836( 1): 112.[citado 2024 maio 06 ] Available from: https://arxiv.org/abs/1701.05201
Vancouver
Dulaney NA, Richardson ND, Gerhartz CJ, Carciofi AC. A Spectroscopic Orbit for the late-type Be star β CMi [Internet]. Astrophysical Journal. 2017 ;836( 1): 112.[citado 2024 maio 06 ] Available from: https://arxiv.org/abs/1701.05201

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