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Artigo de periodico
How Magnetic Activity Alters What We Learn from Stellar Spectra (2020)
Spina, Lorenzo ; Moreno, Jorge Luis Meléndez ; Galarza, Jhon J. Yana
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e GALARZA, Jhon J. Yana. How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab8bd7. Acesso em: 25 jul. 2024.
APA
Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2020). How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/ab8bd7
NLM
Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Vancouver
Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Artigo de periodico
Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc (2020)
Botelho, R. B. ; Milone, A de C. ; Moreno, Jorge Luiz Meléndez ; Alves-Brito, A. ; Spina, L ; Bean, J L
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS
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ABNT
BOTELHO, R. B. et al. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc. Monthly Notices of the Royal Astronomical Society, v. 499, p. 2196-2213, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2917. Acesso em: 25 jul. 2024.
APA
Botelho, R. B., Milone, A. de C., Moreno, J. L. M., Alves-Brito, A., Spina, L., & Bean, J. L. (2020). Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc. Monthly Notices of the Royal Astronomical Society, 499, 2196-2213. doi:10.1093/mnras/staa2917
NLM
Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/staa2917
Vancouver
Botelho RB, Milone A de C, Moreno JLM, Alves-Brito A, Spina L, Bean JL. Carbon, isotopic ratio C-12/C-13, and nitrogen in solar twins: constraints for the chemical evolution of the local disc [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 499 2196-2213.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/staa2917
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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Artigo de periodico
Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation (2018)
Liu, F; Yong, D; Asplund, M; Feltzing, S; Mustill, A. J; Moreno, Jorge Luis Meléndez; Ramírez, I; Lin, J
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: FORMAÇÃO DE ESTRELAS, ABUNDÂNCIA ESTELAR
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ABNT
LIU, F et al. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation. Astronomy & Astrophysics, v. 614, p. A138, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201832701. Acesso em: 25 jul. 2024.
APA
Liu, F., Yong, D., Asplund, M., Feltzing, S., Mustill, A. J., Moreno, J. L. M., et al. (2018). Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation. Astronomy & Astrophysics, 614, A138. doi:10.1051/0004-6361/201832701
NLM
Liu F, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM, Ramírez I, Lin J. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation [Internet]. Astronomy & Astrophysics. 2018 ; 614 A138.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201832701
Vancouver
Liu F, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM, Ramírez I, Lin J. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation [Internet]. Astronomy & Astrophysics. 2018 ; 614 A138.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201832701
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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad190
Artigo de periodico
The chemical homogeneity of sun-like stars in the solar neighborhood (2018)
Bedell, Megan; Bean, Jacob L; Moreno, Jorge Luis Meléndez; Spina, Lorenzo; Ramirez, Ivan; Asplund, Martin; Alves-Brito, Alan; Santos, Leonardo dos; Dreizler, Stefan; Yong, David; Monroe, TalaWanda; Casagrande, Luca
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES
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ABNT
BEDELL, Megan et al. The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, v. 865, n. 1, p. 68-1/68-13, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad908. Acesso em: 25 jul. 2024.
APA
Bedell, M., Bean, J. L., Moreno, J. L. M., Spina, L., Ramirez, I., Asplund, M., et al. (2018). The chemical homogeneity of sun-like stars in the solar neighborhood. Astrophysical Journal, 865( 1), 68-1/68-13. doi:10.3847/1538-4357/aad908
NLM
Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Vancouver
Bedell M, Bean JL, Moreno JLM, Spina L, Ramirez I, Asplund M, Alves-Brito A, Santos L dos, Dreizler S, Yong D, Monroe TW, Casagrande L. The chemical homogeneity of sun-like stars in the solar neighborhood [Internet]. Astrophysical Journal. 2018 ; 865( 1): 68-1/68-13.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Artigo de periodico
A formation timescale of the galactic Halo from Mg isotopes in dwarf stars (2018)
Carlos, Marília; Karakas, Amanda I; Cohen, Judith G; Kobayashi, Chiaki; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
CARLOS, Marília et al. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 25 jul. 2024.
APA
Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
NLM
Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Vancouver
Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Artigo de periodico
The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild (2018)
Cain, Madelyn; Frebel, Anna; Gull, Maude; Ji, Alexander P; Placco, Vinicius M; Beers, Timothy C; Moreno, Jorge Luis Meléndez; Ezzeddine, Rana; Casey, Andrew R; Hansen, Terese T; Roederer, Ian U; Sakari, Charli
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, REAÇÕES NUCLEARES
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ABNT
CAIN, Madelyn et al. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, v. 864, n. 1, p. 43-1/43-12, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 25 jul. 2024.
APA
Cain, M., Frebel, A., Gull, M., Ji, A. P., Placco, V. M., Beers, T. C., et al. (2018). The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild. Astrophysical Journal, 864( 1), 43-1/43-12. doi:10.3847/1538-4357/aad37d
NLM
Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Vancouver
Cain M, Frebel A, Gull M, Ji AP, Placco VM, Beers TC, Moreno JLM, Ezzeddine R, Casey AR, Hansen TT, Roederer IU, Sakari C. The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars-One Strong, One Moderate, and One Mild [Internet]. Astrophysical Journal. 2018 ; 864( 1): 43-1/43-12.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Artigo de periodico
Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions (2017)
Santos, Leonardo A. dos; Moreno, Jorge Luiz Meléndez; Bedell, Megan; Bean, Jacob L; Spina, Lorenzo; Brito, Alan Alves; Dreizler, Stefan; Ramírez, Iván; Asplund, Martin
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ESTRELAS, ASTROFÍSICA ESTELAR
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ABNT
SANTOS, Leonardo A. dos et al. Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions. Monthly Notices of the Royal Astronomical Society, v. 472, p. 3425-3436, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2199. Acesso em: 25 jul. 2024.
APA
Santos, L. A. dos, Moreno, J. L. M., Bedell, M., Bean, J. L., Spina, L., Brito, A. A., et al. (2017). Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions. Monthly Notices of the Royal Astronomical Society, 472, 3425-3436. doi:10.1093/mnras/stx2199
NLM
Santos LA dos, Moreno JLM, Bedell M, Bean JL, Spina L, Brito AA, Dreizler S, Ramírez I, Asplund M. Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 472 3425-3436.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stx2199
Vancouver
Santos LA dos, Moreno JLM, Bedell M, Bean JL, Spina L, Brito AA, Dreizler S, Ramírez I, Asplund M. Spectroscopic binaries in the Solar Twin Planet Search program: from substellar-mass to M dwarf companions [Internet]. Monthly Notices of the Royal Astronomical Society. 2017 ; 472 3425-3436.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stx2199
Artigo de periodico
Sc and neutron-capture abundances in Galactic low- and high-α field halo stars (2017)
Fishlock, C. K; Yong, D; Karakas, A. I; Alves-Brito, A; Moreno, Jorge Luiz Meléndez; Nissen, P E; Kobayashi, C; Casey, R
Source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS
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ABNT
FISHLOCK, C. K et al. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 466, p. 4672-4682, 2017Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx047. Acesso em: 25 jul. 2024.
APA
Fishlock, C. K., Yong, D., Karakas, A. I., Alves-Brito, A., Moreno, J. L. M., Nissen, P. E., et al. (2017). Sc and neutron-capture abundances in Galactic low- and high-α field halo stars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 466, 4672-4682. doi:10.1093/mnras/stx047
NLM
Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stx047
Vancouver
Fishlock CK, Yong D, Karakas AI, Alves-Brito A, Moreno JLM, Nissen PE, Kobayashi C, Casey R. Sc and neutron-capture abundances in Galactic low- and high-α field halo stars [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2017 ;466 4672-4682.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stx047
Artigo de periodico
Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization (2017)
Bedell, Megan; Bean, Jacob L; Moreno, Jorge Luiz Meléndez; Mills, Sean M.; Fabrycky, Daniel C; Freitas, Fabrício C; Ramírez, Iván; Asplund, Martin; Liu, Fan; Yong, David
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, PLANETAS
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ABNT
BEDELL, Megan et al. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, v. 839, p. 94. 2017, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6a1d. Acesso em: 25 jul. 2024.
APA
Bedell, M., Bean, J. L., Moreno, J. L. M., Mills, S. M., Fabrycky, D. C., Freitas, F. C., et al. (2017). Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, 839, 94. 2017. doi:10.3847/1538-4357/aa6a1d
NLM
Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
Vancouver
Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
Trabalho de evento-resumo
The [Y/Mg] clock:: estimating stellar ages of solar-type stars (2016)
Tucci, M; Meléndez Moreno, Jorge Luis; Ramírez, Ivan; Bedell, Megan; Bean, Jacob; Asplund, Martin
Source: ASOS -12. Conference titles: International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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ABNT
TUCCI, M et al. The [Y/Mg] clock:: estimating stellar ages of solar-type stars. 2016, Anais.. São Paulo: IAG/USP, 2016. . Acesso em: 25 jul. 2024.
APA
Tucci, M., Meléndez Moreno, J. L., Ramírez, I., Bedell, M., Bean, J., & Asplund, M. (2016). The [Y/Mg] clock:: estimating stellar ages of solar-type stars. In ASOS -12. São Paulo: IAG/USP.
NLM
Tucci M, Meléndez Moreno JL, Ramírez I, Bedell M, Bean J, Asplund M. The [Y/Mg] clock:: estimating stellar ages of solar-type stars. ASOS -12. 2016 ;[citado 2024 jul. 25 ]
Vancouver
Tucci M, Meléndez Moreno JL, Ramírez I, Bedell M, Bean J, Asplund M. The [Y/Mg] clock:: estimating stellar ages of solar-type stars. ASOS -12. 2016 ;[citado 2024 jul. 25 ]
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, 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. 590, p. A66/1-A66/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526643. Acesso em: 25 jul. 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, 590, A66/1-A66/8. 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 ; 590 A66/1-A66/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201526643
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 ; 590 A66/1-A66/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201526643
Artigo de periodico
First high-precision differential abundance analysis of extremely metal-poor stars (2016)
Reggiani, Henrique; Moreno, Jorge Luiz Meléndez; Yong, David; Ramírez, Ivan; Asplund, Martin
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
REGGIANI, Henrique et al. First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, v. 586, p. A67/1-A67/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527439. Acesso em: 25 jul. 2024.
APA
Reggiani, H., Moreno, J. L. M., Yong, D., Ramírez, I., & Asplund, M. (2016). First high-precision differential abundance analysis of extremely metal-poor stars. Astronomy & Astrophysics, 586, A67/1-A67/8. doi:10.1051/0004-6361/201527439
NLM
Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201527439
Vancouver
Reggiani H, Moreno JLM, Yong D, Ramírez I, Asplund M. First high-precision differential abundance analysis of extremely metal-poor stars [Internet]. Astronomy & Astrophysics. 2016 ; 586 A67/1-A67/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201527439
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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stw247
Artigo de periodico
The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars (2016)
Santos, Leonardo A. dos; Moreno, Jorge Luiz Meléndez; Nascimento Júnior, José Dias do; Bedell, Megan; Ramírez, Iván; Bean, Jacob L; Asplund, Martin; Spina, Lorenzo; Dreizler, Stefan; Brito, Alan Alves; Casagrande, Luca
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: SOL, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS, Leonardo A. dos et al. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, v. 592, p. A156/1-A156/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628558. Acesso em: 25 jul. 2024.
APA
Santos, L. A. dos, Moreno, J. L. M., Nascimento Júnior, J. D. do, Bedell, M., Ramírez, I., Bean, J. L., et al. (2016). The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, 592, A156/1-A156/8. doi:10.1051/0004-6361/201628558
NLM
Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201628558
Vancouver
Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201628558
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
Artigo de periodico
The detailed chemical composition of the terrestrial planet host Kepler-10 (2016)
Liu, F; Yong, D; Asplund, M; Ramírez, I; Moreno, Jorge Luiz Meléndez; Gustafsson, B; Howes, M. J; Roederer, I. U; Lambert, D. L; Bensby, T
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LIU, F et al. The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2636-2646, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2821. Acesso em: 25 jul. 2024.
APA
Liu, F., Yong, D., Asplund, M., Ramírez, I., Moreno, J. L. M., Gustafsson, B., et al. (2016). The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, 456, 2636-2646. doi:10.1093/mnras/stv2821
NLM
Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stv2821
Vancouver
Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM, Gustafsson B, Howes MJ, Roederer IU, Lambert DL, Bensby T. The detailed chemical composition of the terrestrial planet host Kepler-10 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 456 2636-2646.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stv2821
Artigo de periodico
High-precision analysis of the solar twin HIP 100963 (2016)
Galarza, Jhon Yana; Moreno, Jorge Luiz Meléndez; Ramírez, Ivan; Yong, David; Karakas, Amanda I; Asplund, Martin; Liu, Fan
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, PLANETAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GALARZA, Jhon Yana et al. High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, v. 589, p. A17/1-A17/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527912. Acesso em: 25 jul. 2024.
APA
Galarza, J. Y., Moreno, J. L. M., Ramírez, I., Yong, D., Karakas, A. I., Asplund, M., & Liu, F. (2016). High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, 589, A17/1-A17/8. doi:10.1051/0004-6361/201527912
NLM
Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201527912
Vancouver
Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1051/0004-6361/201527912
Artigo de periodico
GRACES observations of young [α/Fe]-rich stars (2016)
Yong, David; Casagrande, Luca; Venn, Kim A; Chené, André-Nicolas; Keown, Jared; Malo, Lison; Martioli, Eder; Moreno, Jorge Luiz Meléndez
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
YONG, David et al. GRACES observations of young [α/Fe]-rich stars. Monthly Notices of the Royal Astronomical Society, v. 459, p. 487-495, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw676. Acesso em: 25 jul. 2024.
APA
Yong, D., Casagrande, L., Venn, K. A., Chené, A. -N., Keown, J., Malo, L., et al. (2016). GRACES observations of young [α/Fe]-rich stars. Monthly Notices of the Royal Astronomical Society, 459, 487-495. doi:10.1093/mnras/stw676
NLM
Yong D, Casagrande L, Venn KA, Chené A-N, Keown J, Malo L, Martioli E, Moreno JLM. GRACES observations of young [α/Fe]-rich stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 459 487-495.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stw676
Vancouver
Yong D, Casagrande L, Venn KA, Chené A-N, Keown J, Malo L, Martioli E, Moreno JLM. GRACES observations of young [α/Fe]-rich stars [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 459 487-495.[citado 2024 jul. 25 ] Available from: https://doi.org/10.1093/mnras/stw676

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