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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: 31 out. 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 out. 31 ] 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 out. 31 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Artigo de periodico
Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 (2020)
Nascimento J.-D. do ; Almeida, L. de ; Velloso, E. N ; Anthony, F.; Costa, J. S. da; Castro, M; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
NASCIMENTO J.-D. DO, et al. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, v. 898, p. 173 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab9c16. Acesso em: 31 out. 2024.
APA
Nascimento J.-D. do,, Almeida, L. de, Velloso, E. N., Anthony, F., Costa, J. S. da, Castro, M., & Moreno, J. L. M. (2020). Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, 898, 173 2020. doi:10.3847/1538-4357/ab9c16
NLM
Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 out. 31 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
Vancouver
Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 out. 31 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
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: 31 out. 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 out. 31 ] 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 out. 31 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Artigo de periodico
The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun (2020)
Lorenzo-Oliveira, Diego ; Moreno, Jorge Luis Meléndez ; Ponte, Geisa ; Galarza, Jhon J. Yana
Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG
Subjects: ABUNDANCIA ESTELAR, FORMAÇÃO DE ESTRELAS
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ABNT
LORENZO-OLIVEIRA, Diego et al. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun. Monthly Notices of the Royal Astronomical Society Letters, v. 495, p. L61-L65, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa2917. Acesso em: 31 out. 2024.
APA
Lorenzo-Oliveira, D., Moreno, J. L. M., Ponte, G., & Galarza, J. J. Y. (2020). The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun. Monthly Notices of the Royal Astronomical Society Letters, 495, L61-L65. doi:10.1093/mnras/staa2917
NLM
Lorenzo-Oliveira D, Moreno JLM, Ponte G, Galarza JJY. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2020 ; 495 L61-L65.[citado 2024 out. 31 ] Available from: https://doi.org/10.1093/mnras/staa2917
Vancouver
Lorenzo-Oliveira D, Moreno JLM, Ponte G, Galarza JJY. The ancient main-sequence solar proxy HIP 102152 unveils the activity and rotational fate of our Sun [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2020 ; 495 L61-L65.[citado 2024 out. 31 ] Available from: https://doi.org/10.1093/mnras/staa2917
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: 31 out. 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 out. 31 ] 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 out. 31 ] 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: 31 out. 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 out. 31 ] 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 out. 31 ] 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: 31 out. 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 out. 31 ] 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 out. 31 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Artigo de periodico
The temporal evolution of neutron-capture elements in the Galactic discs (2018)
Spina, Lorenzo; Moreno, Jorge Luis Meléndez; Alves-Brito, Alan
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)
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ABNT
SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e ALVES-BRITO, Alan. The temporal evolution of neutron-capture elements in the Galactic discs. Monthly Notices of the Royal Astronomical Society, v. 474, n. 2, p. 2580-2593, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2938. Acesso em: 31 out. 2024.
APA
Spina, L., Moreno, J. L. M., & Alves-Brito, A. (2018). The temporal evolution of neutron-capture elements in the Galactic discs. Monthly Notices of the Royal Astronomical Society, 474( 2), 2580-2593. doi:10.1093/mnras/stx2938
NLM
Spina L, Moreno JLM, Alves-Brito A. The temporal evolution of neutron-capture elements in the Galactic discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 474( 2): 2580-2593.[citado 2024 out. 31 ] Available from: https://doi.org/10.1093/mnras/stx2938
Vancouver
Spina L, Moreno JLM, Alves-Brito A. The temporal evolution of neutron-capture elements in the Galactic discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 474( 2): 2580-2593.[citado 2024 out. 31 ] Available from: https://doi.org/10.1093/mnras/stx2938
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: 31 out. 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 out. 31 ] 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 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201832701
Artigo de periodico
Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 (2018)
Reggiani, Henrique; Moreno, Jorge Luis Meléndez
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS
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ABNT
REGGIANI, Henrique e MORENO, Jorge Luis Meléndez. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440. Monthly Notices of the Royal Astronomical Society, v. 475, n. 3, p. 3502-3510, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty104. Acesso em: 31 out. 2024.
APA
Reggiani, H., & Moreno, J. L. M. (2018). Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440. Monthly Notices of the Royal Astronomical Society, 475( 3), 3502-3510. doi:10.1093/mnras/sty104
NLM
Reggiani H, Moreno JLM. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 3502-3510.[citado 2024 out. 31 ] Available from: https://doi.org/10.1093/mnras/sty104
Vancouver
Reggiani H, Moreno JLM. Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440 [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 3502-3510.[citado 2024 out. 31 ] Available from: https://doi.org/10.1093/mnras/sty104
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: 31 out. 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 out. 31 ] 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 out. 31 ] 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: 31 out. 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 out. 31 ] 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 out. 31 ] 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: 31 out. 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 out. 31 ] 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 out. 31 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Artigo de periodico
Modelling the solar twin 18 Scorpii (2018)
Bazot, M; Creevey, O; Christensen-Dalsgaard, J; Moreno, Jorge Luis Meléndez
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, EVOLUÇÃO ESTELAR
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ABNT
BAZOT, M et al. Modelling the solar twin 18 Scorpii. Astronomy & Astrophysics, v. 619, p. A172, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834058. Acesso em: 31 out. 2024.
APA
Bazot, M., Creevey, O., Christensen-Dalsgaard, J., & Moreno, J. L. M. (2018). Modelling the solar twin 18 Scorpii. Astronomy & Astrophysics, 619, A172. doi:10.1051/0004-6361/201834058
NLM
Bazot M, Creevey O, Christensen-Dalsgaard J, Moreno JLM. Modelling the solar twin 18 Scorpii [Internet]. Astronomy & Astrophysics. 2018 ; 619 A172.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201834058
Vancouver
Bazot M, Creevey O, Christensen-Dalsgaard J, Moreno JLM. Modelling the solar twin 18 Scorpii [Internet]. Astronomy & Astrophysics. 2018 ; 619 A172.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201834058
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: 31 out. 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 out. 31 ] 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 out. 31 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
Artigo de periodico
Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** (2017)
Bensby, T; Moreno, Jorge Luis Meléndez
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BENSBY, T e MORENO, Jorge Luis Meléndez. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, v. 605, p. 89, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730560. Acesso em: 31 out. 2024.
APA
Bensby, T., & Moreno, J. L. M. (2017). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,**. Astronomy & Astrophysics, 605, 89. doi:10.1051/0004-6361/201730560
NLM
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201730560
Vancouver
Bensby T, Moreno JLM. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - VI Age and abundances structure of the stellar populations in the central sub-kpc of the milky way *,** [Internet]. Astronomy & Astrophysics. 2017 ; 605 89.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201730560
Artigo de periodico
G64-12 and G64-37 are carbon-enhanced metal-poor stars (2016)
Placco, Vinicius M; Beers, Timothy C; Reggiani, Henrique; Moreno, Jorge Luis Meléndez
Source: The Astrophysical Journal Letters. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
PLACCO, Vinicius M et al. G64-12 and G64-37 are carbon-enhanced metal-poor stars. The Astrophysical Journal Letters, 2016Tradução . . Disponível em: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf. Acesso em: 31 out. 2024.
APA
Placco, V. M., Beers, T. C., Reggiani, H., & Moreno, J. L. M. (2016). G64-12 and G64-37 are carbon-enhanced metal-poor stars. The Astrophysical Journal Letters. doi:10.3847/2041-8205/829/2/L24
NLM
Placco VM, Beers TC, Reggiani H, Moreno JLM. G64-12 and G64-37 are carbon-enhanced metal-poor stars [Internet]. The Astrophysical Journal Letters. 2016 ;[citado 2024 out. 31 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
Vancouver
Placco VM, Beers TC, Reggiani H, Moreno JLM. G64-12 and G64-37 are carbon-enhanced metal-poor stars [Internet]. The Astrophysical Journal Letters. 2016 ;[citado 2024 out. 31 ] Available from: http://iopscience.iop.org/article/10.3847/2041-8205/829/2/L24/pdf
Trabalho de evento-resumo
Precision abundances (2016)
Moreno, Jorge Luis Meléndez
Source: ASOS -12. Conference titles: International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas. Unidade: IAG
Subjects: ABUNDÂNCIAS (ASTRONOMIA), ASTROFÍSICA ESTELAR
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
MORENO, Jorge Luis Meléndez. Precision abundances. 2016, Anais.. São Paulo: IAG/USP, 2016. . Acesso em: 31 out. 2024.
APA
Moreno, J. L. M. (2016). Precision abundances. In ASOS -12. São Paulo: IAG/USP.
NLM
Moreno JLM. Precision abundances. ASOS -12. 2016 ;[citado 2024 out. 31 ]
Vancouver
Moreno JLM. Precision abundances. ASOS -12. 2016 ;[citado 2024 out. 31 ]
Artigo de periodico
The solar twin planet search: II. A Jupiter twin around a solar twin (2015)
Bedell, M; Moreno, Jorge Luis Meléndez; Bean, J. L; Ramírez, I; Asplund, M; Alves-Brito, A; Casagrande, L; Dreizler, S; Monroe, T; Spina, L; Tucci Maia, Mi
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, ATIVIDADE ESTELAR, VELOCIDADE
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
BEDELL, M et al. The solar twin planet search: II. A Jupiter twin around a solar twin. Astronomy & Astrophysics, v. 581, p. A34/1-A34/7, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525748. Acesso em: 31 out. 2024.
APA
Bedell, M., Moreno, J. L. M., Bean, J. L., Ramírez, I., Asplund, M., Alves-Brito, A., et al. (2015). The solar twin planet search: II. A Jupiter twin around a solar twin. Astronomy & Astrophysics, 581, A34/1-A34/7. doi:10.1051/0004-6361/201525748
NLM
Bedell M, Moreno JLM, Bean JL, Ramírez I, Asplund M, Alves-Brito A, Casagrande L, Dreizler S, Monroe T, Spina L, Tucci Maia M. The solar twin planet search: II. A Jupiter twin around a solar twin [Internet]. Astronomy & Astrophysics. 2015 ; 581 A34/1-A34/7.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201525748
Vancouver
Bedell M, Moreno JLM, Bean JL, Ramírez I, Asplund M, Alves-Brito A, Casagrande L, Dreizler S, Monroe T, Spina L, Tucci Maia M. The solar twin planet search: II. A Jupiter twin around a solar twin [Internet]. Astronomy & Astrophysics. 2015 ; 581 A34/1-A34/7.[citado 2024 out. 31 ] Available from: https://doi.org/10.1051/0004-6361/201525748
Artigo de periodico
Chemical abundances and physical parameters of HII regions in the Magellanic Clouds (2015)
Carlos Reyes, R. E; Navarro, F. A. R; Moreno, Jorge Luis Meléndez; Steiner, João Evangelista; Elizalde, F
Source: Revista Mexicana de Astronomía y Astrofísica. Unidade: IAG
Subjects: REGIÕES HII (ASTRONOMIA), NUVENS DE MAGALHÃES, ANÁLISE DE DADOS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
CARLOS REYES, R. E et al. Chemical abundances and physical parameters of HII regions in the Magellanic Clouds. Revista Mexicana de Astronomía y Astrofísica, v. 51, p. 133-145, 2015Tradução . . Acesso em: 31 out. 2024.
APA
Carlos Reyes, R. E., Navarro, F. A. R., Moreno, J. L. M., Steiner, J. E., & Elizalde, F. (2015). Chemical abundances and physical parameters of HII regions in the Magellanic Clouds. Revista Mexicana de Astronomía y Astrofísica, 51, 133-145.
NLM
Carlos Reyes RE, Navarro FAR, Moreno JLM, Steiner JE, Elizalde F. Chemical abundances and physical parameters of HII regions in the Magellanic Clouds. Revista Mexicana de Astronomía y Astrofísica. 2015 ; 51 133-145.[citado 2024 out. 31 ]
Vancouver
Carlos Reyes RE, Navarro FAR, Moreno JLM, Steiner JE, Elizalde F. Chemical abundances and physical parameters of HII regions in the Magellanic Clouds. Revista Mexicana de Astronomía y Astrofísica. 2015 ; 51 133-145.[citado 2024 out. 31 ]

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