ReP USP - Resultado da busca

Artigo de periodico
The detailed chemical composition of the terrestrial planet host Kepler-10 (2016)
Liu, F; Yong, D; Asplund, M; Ramírez, I; Moreno, Jorge Luiz Meléndez; Gustafsson, B; Howes, M. J; Roederer, I. U; Lambert, D. L; Bensby, T
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
LIU, F et al. The detailed chemical composition of the terrestrial planet host Kepler-10. Monthly Notices of the Royal Astronomical Society, v. 456, p. 2636-2646, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stv2821. Acesso em: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Trabalho de evento
The chemical evolution of the Galactic Bulge seen through micro-lensing events (2012)
Feltzing, S; Bensby, T; Moreno, Jorge Luiz Meléndez; Adén, D; Asplund, M; Gould, A; Johnson, J; Lucatello, S; Gal-Yam, A
Source: EPJ Web of Conferences, 19. Conference titles: Assembling the Puzzle of the Milky Way. Unidade: IAG
Subjects: FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, GALÁXIA (VIA LÁCTEA), ASTROQUÍMICA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
FELTZING, S et al. The chemical evolution of the Galactic Bulge seen through micro-lensing events. 2012, Anais.. Les Ulis: EPD Sciences, 2012. Disponível em: https://doi.org/10.1051/epjconf/20121906002. Acesso em: 23 abr. 2024.
APA
Feltzing, S., Bensby, T., Moreno, J. L. M., Adén, D., Asplund, M., Gould, A., et al. (2012). The chemical evolution of the Galactic Bulge seen through micro-lensing events. In EPJ Web of Conferences, 19. Les Ulis: EPD Sciences. doi:10.1051/epjconf/20121906002
NLM
Feltzing S, Bensby T, Moreno JLM, Adén D, Asplund M, Gould A, Johnson J, Lucatello S, Gal-Yam A. The chemical evolution of the Galactic Bulge seen through micro-lensing events [Internet]. EPJ Web of Conferences, 19. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1051/epjconf/20121906002
Vancouver
Feltzing S, Bensby T, Moreno JLM, Adén D, Asplund M, Gould A, Johnson J, Lucatello S, Gal-Yam A. The chemical evolution of the Galactic Bulge seen through micro-lensing events [Internet]. EPJ Web of Conferences, 19. 2012 ;[citado 2024 abr. 23 ] Available from: https://doi.org/10.1051/epjconf/20121906002
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 590, p. A66/1-A66/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526643. Acesso em: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: 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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1093/mnras/staa2917
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: 23 abr. 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 abr. 23 ]
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 abr. 23 ]
Artigo de periodico
The UBV '(RI) IND. C' colors of the sun (2012)
Ramírez, I; Michel, R; Sefako, R; Maia, M. Tucci; Schuster, W. J; van Wyk, F; Meléndez Moreno, Jorge Luis; Casagrande, L; Castilho, B. V
Source: The Astrophysical Journal. Unidade: IAG
Subjects: ESTRELAS, SOL, FOTOMETRIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RAMÍREZ, I et al. The UBV '(RI) IND. C' colors of the sun. The Astrophysical Journal, v. 752, p. 5/1-5/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/752/1/5. Acesso em: 23 abr. 2024.
APA
Ramírez, I., Michel, R., Sefako, R., Maia, M. T., Schuster, W. J., van Wyk, F., et al. (2012). The UBV '(RI) IND. C' colors of the sun. The Astrophysical Journal, 752, 5/1-5/13. doi:10.1088/0004-637X/752/1/5
NLM
Ramírez I, Michel R, Sefako R, Maia MT, Schuster WJ, van Wyk F, Meléndez Moreno JL, Casagrande L, Castilho BV. The UBV '(RI) IND. C' colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 752 5/1-5/13.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1088/0004-637X/752/1/5
Vancouver
Ramírez I, Michel R, Sefako R, Maia MT, Schuster WJ, van Wyk F, Meléndez Moreno JL, Casagrande L, Castilho BV. The UBV '(RI) IND. C' colors of the sun [Internet]. The Astrophysical Journal. 2012 ; 752 5/1-5/13.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1088/0004-637X/752/1/5
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)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.1017/S1743921313006546
Artigo de periodico
The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars (2016)
Santos, Leonardo A. dos; Moreno, Jorge Luiz Meléndez; Nascimento Júnior, José Dias do; Bedell, Megan; Ramírez, Iván; Bean, Jacob L; Asplund, Martin; Spina, Lorenzo; Dreizler, Stefan; Brito, Alan Alves; Casagrande, Luca
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: SOL, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS, Leonardo A. dos et al. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, v. 592, p. A156/1-A156/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628558. Acesso em: 23 abr. 2024.
APA
Santos, L. A. dos, Moreno, J. L. M., Nascimento Júnior, J. D. do, Bedell, M., Ramírez, I., Bean, J. L., et al. (2016). The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, 592, A156/1-A156/8. doi:10.1051/0004-6361/201628558
NLM
Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1051/0004-6361/201628558
Vancouver
Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1051/0004-6361/201628558
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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] 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: 23 abr. 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 abr. 23 ] 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 abr. 23 ] Available from: https://doi.org/10.3847/1538-4357/aad37d

USP Schools

ReP

Filtros

Document Types

Authors

USP affiliated authors

Date published

Subjects

Source title

Publisher

Conference titles

Countries/Territories

Normalized affiliation

Non normalized affiliation

Countries of institutions of collaboration