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Artigo de periodico
The hubble Space Telescope UV legacy survey of galactic globular clusters: XVI. The helium abundance of multiple populations (2018)
Milone, A. P; Marino, A. F; Renzini, A; Barbuy, Beatriz Leonor Silveira
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES
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ABNT
MILONE, A. P et al. The hubble Space Telescope UV legacy survey of galactic globular clusters: XVI. The helium abundance of multiple populations. Monthly Notices of the Royal Astronomical Society, v. 481, n. 4, p. 5098-5122, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty2573. Acesso em: 09 maio 2024.
APA
Milone, A. P., Marino, A. F., Renzini, A., & Barbuy, B. L. S. (2018). The hubble Space Telescope UV legacy survey of galactic globular clusters: XVI. The helium abundance of multiple populations. Monthly Notices of the Royal Astronomical Society, 481( 4), 5098-5122. doi:10.1093/mnras/sty2573
NLM
Milone AP, Marino AF, Renzini A, Barbuy BLS. The hubble Space Telescope UV legacy survey of galactic globular clusters: XVI. The helium abundance of multiple populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 481( 4): 5098-5122.[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnras/sty2573
Vancouver
Milone AP, Marino AF, Renzini A, Barbuy BLS. The hubble Space Telescope UV legacy survey of galactic globular clusters: XVI. The helium abundance of multiple populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 481( 4): 5098-5122.[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnras/sty2573
Artigo de periodico
The future of the Sun: an evolved solar twin revealed by CoRoT (2013)
Nascimento Júnior, J.-D. do; Takeda, Y; Moreno, Jorge Luis Meléndez; Costa, J. S. da; Mello, G. F. Porto de; Castro, M
Source: The Astrophysical Journal Letters. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS, SOL
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NASCIMENTO JÚNIOR, J.-D. do et al. The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, v. 771, p. L31/1-L31/5, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/771/2/L31. Acesso em: 09 maio 2024.
APA
Nascimento Júnior, J. -D. do, Takeda, Y., Moreno, J. L. M., Costa, J. S. da, Mello, G. F. P. de, & Castro, M. (2013). The future of the Sun: an evolved solar twin revealed by CoRoT. The Astrophysical Journal Letters, 771, L31/1-L31/5. doi:10.1088/2041-8205/771/2/L31
NLM
Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 maio 09 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
Vancouver
Nascimento Júnior J-D do, Takeda Y, Moreno JLM, Costa JS da, Mello GFP de, Castro M. The future of the Sun: an evolved solar twin revealed by CoRoT [Internet]. The Astrophysical Journal Letters. 2013 ; 771 L31/1-L31/5.[citado 2024 maio 09 ] Available from: https://doi.org/10.1088/2041-8205/771/2/L31
Artigo de periodico
The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 (2019)
Galarza, Jhon Yana; Meléndez, Jorge; Lorenzo-Oliveira, Diego; Reggiani, Henrique; Carlos, Marília; Ponte, Geisa
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESPECTROMETRIA, ATMOSFERAS ESTELARES
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ABNT
GALARZA, Jhon Yana et al. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, v. 490, p. L86-L90, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slz153. Acesso em: 09 maio 2024.
APA
Galarza, J. Y., Meléndez, J., Lorenzo-Oliveira, D., Reggiani, H., Carlos, M., & Ponte, G. (2019). The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, 490, L86-L90. doi:10.1093/mnrasl/slz153
NLM
Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnrasl/slz153
Vancouver
Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnrasl/slz153
Artigo de periodico
The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system (2015)
Ramírez, I; Khanal, S; Aleo, P; Sobotka, A; Liu, F; Casagrande, L; Moreno, Jorge Luiz Meléndez; Yong, D; Lambert, D. L; Asplund, M
Source: The Astrophysical Journal. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS
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ABNT
RAMÍREZ, I et al. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, v. 808, p. 13/1-13/14, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/808/1/13. Acesso em: 09 maio 2024.
APA
Ramírez, I., Khanal, S., Aleo, P., Sobotka, A., Liu, F., Casagrande, L., et al. (2015). The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system. The Astrophysical Journal, 808, 13/1-13/14. doi:10.1088/0004-637X/808/1/13
NLM
Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 maio 09 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
Vancouver
Ramírez I, Khanal S, Aleo P, Sobotka A, Liu F, Casagrande L, Moreno JLM, Yong D, Lambert DL, Asplund M. The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system [Internet]. The Astrophysical Journal. 2015 ; 808 13/1-13/14.[citado 2024 maio 09 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
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
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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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.1093/mnras/stv2821
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Artigo de periodico
The chemical compositions of solar twins in the open cluster M67 (2016)
Asplund, F; Asplund, M; Yong, D; Moreno, Jorge Luiz Meléndez; Ramírez, I; Karakas, A. I; Carlos, M; Marino, A. F
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
ASPLUND, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, v. 463, p. 696-704, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 09 maio 2024.
APA
Asplund, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 463, 696-704. doi:10.1093/mnras/stw2045
NLM
Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnras/stw2045
Vancouver
Asplund F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 463 696-704.[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnras/stw2045
Artigo de periodico
The chemical compositions of solar twins in the open cluster M67 (2016)
Liu, F; Asplund, Martin; Yong, D; Moreno, Jorge Luiz Meléndez; Ramírez, Iván; Karakas, A. I; Carlos, M; Marino, A. F
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assunto: ABUNDÂNCIA ESTELAR
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ABNT
LIU, F et al. The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw2045. Acesso em: 09 maio 2024.
APA
Liu, F., Asplund, M., Yong, D., Moreno, J. L. M., Ramírez, I., Karakas, A. I., et al. (2016). The chemical compositions of solar twins in the open cluster M67. Monthly Notices of the Royal Astronomical Society. doi:10.1093/mnras/stw2045
NLM
Liu F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnras/stw2045
Vancouver
Liu F, Asplund M, Yong D, Moreno JLM, Ramírez I, Karakas AI, Carlos M, Marino AF. The chemical compositions of solar twins in the open cluster M67 [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ;[citado 2024 maio 09 ] Available from: https://doi.org/10.1093/mnras/stw2045
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: 09 maio 2024.
APA
Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.1051/0004-6361/201526643
Artigo de periodico
The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios (2016)
Thygesen, A. O; Sbordone, L; Ludwig, H.-G; Ventura, P; Yong, D; Collet, R; Christlieb, N; Moreno, Jorge Luiz Meléndez; Zaggia, S
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA
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ABNT
THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 09 maio 2024.
APA
Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 588, A66. doi:10.1051/0004-6361/201526643
NLM
Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 maio 09 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
Vancouver
Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 maio 09 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
Artigo de periodico
The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns (2014)
Thygesen, A. O; Sbordone, L; Andrievsky, S; Korotin, S.; Yong, D; Zaggia, S; Ludwig, H.-G; Collet, R; Asplund, M; Ventura, P; D'Antona, F; Moreno, Jorge Luiz Meléndez; D'Ercole, A
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA
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ABNT
THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns. Astronomy & Astrophysics, v. 572, p. A108/1-A108/21, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424533. Acesso em: 09 maio 2024.
APA
Thygesen, A. O., Sbordone, L., Andrievsky, S., Korotin, S., Yong, D., Zaggia, S., et al. (2014). The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns. Astronomy & Astrophysics, 572, A108/1-A108/21. doi:10.1051/0004-6361/201424533
NLM
Thygesen AO, Sbordone L, Andrievsky S, Korotin S, Yong D, Zaggia S, Ludwig H-G, Collet R, Asplund M, Ventura P, D'Antona F, Moreno JLM, D'Ercole A. The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns [Internet]. Astronomy & Astrophysics. 2014 ; 572 A108/1-A108/21.[citado 2024 maio 09 ] Available from: https://doi.org/10.1051/0004-6361/201424533
Vancouver
Thygesen AO, Sbordone L, Andrievsky S, Korotin S, Yong D, Zaggia S, Ludwig H-G, Collet R, Asplund M, Ventura P, D'Antona F, Moreno JLM, D'Ercole A. The chemical composition of red giants in 47 Tucanae: I. Fundamental parameters and chemical abundance patterns [Internet]. Astronomy & Astrophysics. 2014 ; 572 A108/1-A108/21.[citado 2024 maio 09 ] Available from: https://doi.org/10.1051/0004-6361/201424533
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
Trabalho de evento
The Sun: a typical star in the solar neighborhood? (2014)
Moreno, Jorge Luiz Meléndez
Source: Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. Conference titles: IAU Symposium. Unidade: IAG
Subjects: SOL, ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, FORMAÇÃO DO SISTEMA SOLAR, TERRA (PLANETA)
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ABNT
MORENO, Jorge Luiz Meléndez. The Sun: a typical star in the solar neighborhood? 2014, Anais.. Paris: International Astronomical Union, 2014. Disponível em: https://doi.org/10.1017/S1743921313006546. Acesso em: 09 maio 2024.
APA
Moreno, J. L. M. (2014). The Sun: a typical star in the solar neighborhood? In Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. Paris: International Astronomical Union. doi:10.1017/S1743921313006546
NLM
Moreno JLM. The Sun: a typical star in the solar neighborhood? [Internet]. Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. 2014 ;[citado 2024 maio 09 ] Available from: https://doi.org/10.1017/S1743921313006546
Vancouver
Moreno JLM. The Sun: a typical star in the solar neighborhood? [Internet]. Setting the scene for Gaia and LAMOST: Proceedings IAU Symposium n. 298, 2013. 2014 ;[citado 2024 maio 09 ] Available from: https://doi.org/10.1017/S1743921313006546
Artigo de periodico
The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars (2016)
Tucci Maia, M; Ramírez, I; Moreno, Jorge Luiz Meléndez; Bedell, M; Bean, J. L; Asplund, M
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
TUCCI MAIA, M et al. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars. Astronomy & Astrophysics, v. 590, p. A32/1-A32/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527848. Acesso em: 09 maio 2024.
APA
Tucci Maia, M., Ramírez, I., Moreno, J. L. M., Bedell, M., Bean, J. L., & Asplund, M. (2016). The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars. Astronomy & Astrophysics, 590, A32/1-A32/8. doi:10.1051/0004-6361/201527848
NLM
Tucci Maia M, Ramírez I, Moreno JLM, Bedell M, Bean JL, Asplund M. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars [Internet]. Astronomy & Astrophysics. 2016 ; 590 A32/1-A32/8.[citado 2024 maio 09 ] Available from: https://doi.org/10.1051/0004-6361/201527848
Vancouver
Tucci Maia M, Ramírez I, Moreno JLM, Bedell M, Bean JL, Asplund M. The Solar Twin Planet Search: III. The [Y/Mg] clock: estimating stellar ages of solar-type stars [Internet]. Astronomy & Astrophysics. 2016 ; 590 A32/1-A32/8.[citado 2024 maio 09 ] Available from: https://doi.org/10.1051/0004-6361/201527848
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.1051/0004-6361/201527775
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
Artigo de periodico
The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey (2019)
Placco, Vinicius M; Santucci, Rafael M; Rossi, Silvia Cristina Fernandes
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
PLACCO, Vinicius M e SANTUCCI, Rafael M e ROSSI, Silvia Cristina Fernandes. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, v. 870, n. 2, p. 122-1/122-11, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf3b9. Acesso em: 09 maio 2024.
APA
Placco, V. M., Santucci, R. M., & Rossi, S. C. F. (2019). The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, 870( 2), 122-1/122-11. doi:10.3847/1538-4357/aaf3b9
NLM
Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2024 maio 09 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
Vancouver
Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2024 maio 09 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 09 maio 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 maio 09 ] 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 maio 09 ] Available from: https://doi.org/10.3847/1538-4357/aad37d

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