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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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1093/mnras/staa2917
Artigo de periodico
The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars (2020)
Cain,Madelyn ; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
CAIN, Madelyn e MORENO, Jorge Luis Meléndez. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, v. 864, p. 43 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d. Acesso em: 10 jun. 2024.
APA
Cain, M., & Moreno, J. L. M. (2020). The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars. Astrophysical Journal, 864, 43 2020. doi:10.3847/1538-4357/aad37d
NLM
Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2024 jun. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Vancouver
Cain M, Moreno JLM. The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars [Internet]. Astrophysical Journal. 2020 ; 864 43 2020.[citado 2024 jun. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Artigo de periodico
The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* (2020)
Ezzeddine, Rana; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
EZZEDDINE, Rana e MORENO, Jorge Luis Meléndez. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, v. 898, p. 150 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad37d1a. Acesso em: 10 jun. 2024.
APA
Ezzeddine, R., & Moreno, J. L. M. (2020). The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars*. Astrophysical Journal, 898, 150 2020. doi:10.3847/1538-4357/aad37d1a
NLM
Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2024 jun. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
Vancouver
Ezzeddine R, Moreno JLM. The R-Process Alliance: first magellan/MIKE release from the southern search for r-process-enhanced stars* [Internet]. Astrophysical Journal. 2020 ; 898 150 2020.[citado 2024 jun. 10 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
Artigo de periodico
Constraining teh evolutionofstellar rotation using solar twins (2019)
Lorenzo-Oliveira, Diego; Moreno, Jorge Luiz Meléndez; Lichon, S. J; Chanamé, J; Endl, M; Moreno, Jorge Luis Meléndez; Lambert, D. L.
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ASTROFISICA ESTELAR, SOL
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ABNT
LORENZO-OLIVEIRA, Diego et al. Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 10 jun. 2024.
APA
Lorenzo-Oliveira, D., Moreno, J. L. M., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). Constraining teh evolutionofstellar rotation using solar twins. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/slz034
NLM
Lorenzo-Oliveira D, Moreno JLM, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 jun. 10 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Vancouver
Lorenzo-Oliveira D, Moreno JLM, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. Constraining teh evolutionofstellar rotation using solar twins [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 jun. 10 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Artigo de periodico
The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs (2019)
Ramirez; Khanal, S.; Lichon, S. J; Chanamé, J; Endl, M; Moreno, Jorge Luis Meléndez; Lambert, D. L.
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS BINARIAS
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ABNT
RAMIREZ, et al. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, v. 490, p. 2448-2457, 2019Tradução . . Disponível em: https://academic.oup.com/mnras/article/490/2/2448/5583050. Acesso em: 10 jun. 2024.
APA
Ramirez,, Khanal, S., Lichon, S. J., Chanamé, J., Endl, M., Moreno, J. L. M., & Lambert, D. L. (2019). The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs. Monthly Notices of the Royal Astronomical Society, 490, 2448-2457. doi:10.1093/mnras/sty104
NLM
Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 jun. 10 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Vancouver
Ramirez, Khanal S, Lichon SJ, Chanamé J, Endl M, Moreno JLM, Lambert DL. The chemical composition of HIP 34407/HIP 34426 and other twin-star comoving pairs [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 2448-2457.[citado 2024 jun. 10 ] 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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201832701
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] 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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Artigo de periodico
The solar twin planet search: The age - chromospheric activity relation (2018)
Lorenzo-Oliveira, Diego; Freitas, Fabrício C; Moreno, Jorge Luiz Meléndez; Bedell, Megan
Source: Astronomy and Astrophysysics. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR
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ABNT
LORENZO-OLIVEIRA, Diego et al. The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, v. 619, p. A73, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629294. Acesso em: 10 jun. 2024.
APA
Lorenzo-Oliveira, D., Freitas, F. C., Moreno, J. L. M., & Bedell, M. (2018). The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, 619, A73. doi:10.1051/0004-6361/201629294
NLM
Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201629294
Vancouver
Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201629294
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] 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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1093/mnras/stx2199
Artigo de periodico
The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 (2017)
Moreno, Jorge Luiz Meléndez; Bedell, Megan; Bean, Jacob L; Mello, Sylvio Ferras; Galarza, Jhon Yana; Santos, Leonardo dos; Spina, Lorenzo; Maia, Marcelo Tucci
Source: Astronomy and Astrophysysics. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR
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ABNT
MORENO, Jorge Luiz Meléndez et al. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, v. 597, p. A34, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527775. Acesso em: 10 jun. 2024.
APA
Moreno, J. L. M., Bedell, M., Bean, J. L., Mello, S. F., Galarza, J. Y., Santos, L. dos, et al. (2017). The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, 597, A34. doi:10.1051/0004-6361/201527775
NLM
Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527775
Vancouver
Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527775
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 10 jun. 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 jun. 10 ]
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 jun. 10 ]
Artigo de periodico
Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars (2016)
Spina, Lorenzo; Moreno, Jorge Luiz Meléndez; Ramírez, Iván
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 10 jun. 2024.
APA
Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
NLM
Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527429
Vancouver
Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527429
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527439
Artigo de periodico
Serendipitous discovery of the faint solar twin Inti 1 (2016)
Galarza, Jhon Yana; Moreno, Jorge Luiz Meléndez; Cohen, Judith G
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, TERRA (PLANETA), PLANETAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
GALARZA, Jhon Yana e MORENO, Jorge Luiz Meléndez e COHEN, Judith G. Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, v. 589, p. A65/1-A65/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527477. Acesso em: 10 jun. 2024.
APA
Galarza, J. Y., Moreno, J. L. M., & Cohen, J. G. (2016). Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, 589, A65/1-A65/8. doi:10.1051/0004-6361/201527477
NLM
Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527477
Vancouver
Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527477
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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1093/mnras/stw247

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