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Artigo de periodico
The solar twin planet search: The age - chromospheric activity relation (2018)
Lorenzo-Oliveira, Diego; Freitas, Fabrício C; Moreno, Jorge Luiz Meléndez; Bedell, Megan
Source: Astronomy and Astrophysysics. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR
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ABNT
LORENZO-OLIVEIRA, Diego et al. The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, v. 619, p. A73, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629294. Acesso em: 20 jun. 2024.
APA
Lorenzo-Oliveira, D., Freitas, F. C., Moreno, J. L. M., & Bedell, M. (2018). The solar twin planet search: The age - chromospheric activity relation. Astronomy and Astrophysysics, 619, A73. doi:10.1051/0004-6361/201629294
NLM
Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201629294
Vancouver
Lorenzo-Oliveira D, Freitas FC, Moreno JLM, Bedell M. The solar twin planet search: The age - chromospheric activity relation [Internet]. Astronomy and Astrophysysics. 2018 ;619 A73.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201629294
Artigo de periodico
The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 (2017)
Moreno, Jorge Luiz Meléndez; Bedell, Megan; Bean, Jacob L; Mello, Sylvio Ferras; Galarza, Jhon Yana; Santos, Leonardo dos; Spina, Lorenzo; Maia, Marcelo Tucci
Source: Astronomy and Astrophysysics. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR
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ABNT
MORENO, Jorge Luiz Meléndez et al. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, v. 597, p. A34, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527775. Acesso em: 20 jun. 2024.
APA
Moreno, J. L. M., Bedell, M., Bean, J. L., Mello, S. F., Galarza, J. Y., Santos, L. dos, et al. (2017). The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468. Astronomy and Astrophysysics, 597, A34. doi:10.1051/0004-6361/201527775
NLM
Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527775
Vancouver
Moreno JLM, Bedell M, Bean JL, Mello SF, Galarza JY, Santos L dos, Spina L, Maia MT. The Solar Twin Planet Search - V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468 [Internet]. Astronomy and Astrophysysics. 2017 ;597 A34.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527775
Artigo de periodico
Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization (2017)
Bedell, Megan; Bean, Jacob L; Moreno, Jorge Luiz Meléndez; Mills, Sean M.; Fabrycky, Daniel C; Freitas, Fabrício C; Ramírez, Iván; Asplund, Martin; Liu, Fan; Yong, David
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, PLANETAS
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ABNT
BEDELL, Megan et al. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, v. 839, p. 94. 2017, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aa6a1d. Acesso em: 20 jun. 2024.
APA
Bedell, M., Bean, J. L., Moreno, J. L. M., Mills, S. M., Fabrycky, D. C., Freitas, F. C., et al. (2017). Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization. Astrophysical Journal, 839, 94. 2017. doi:10.3847/1538-4357/aa6a1d
NLM
Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 jun. 20 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
Vancouver
Bedell M, Bean JL, Moreno JLM, Mills SM, Fabrycky DC, Freitas FC, Ramírez I, Asplund M, Liu F, Yong D. Kepler-11 is a Solar Twin: Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization [Internet]. Astrophysical Journal. 2017 ; 839 94. 2017.[citado 2024 jun. 20 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
Artigo de periodico
Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei (2017)
Storchi-Bergmann, Thaisa; Schimoia, Jaderson S; Peterson, B M; Elvis, Martin; Denney, K.D; Eracleous, M; Silva, Rodrigo Nemmen da
Source: Astrophysical Journal (Online). Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, PLANETAS
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ABNT
STORCHI-BERGMANN, Thaisa et al. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei. Astrophysical Journal (Online), v. 835, n. 2, p. 236, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/2/236. Acesso em: 20 jun. 2024.
APA
Storchi-Bergmann, T., Schimoia, J. S., Peterson, B. M., Elvis, M., Denney, K. D., Eracleous, M., & Silva, R. N. da. (2017). Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei. Astrophysical Journal (Online), 835( 2), 236. doi:10.3847/1538-4357/835/2/236
NLM
Storchi-Bergmann T, Schimoia JS, Peterson BM, Elvis M, Denney KD, Eracleous M, Silva RN da. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei [Internet]. Astrophysical Journal (Online). 2017 ;835( 2): 236.[citado 2024 jun. 20 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
Vancouver
Storchi-Bergmann T, Schimoia JS, Peterson BM, Elvis M, Denney KD, Eracleous M, Silva RN da. Double-Peaked Profiles: Ubiquitous Signatures of Disks in the Broad Emission Lines of Active Galactic Nuclei [Internet]. Astrophysical Journal (Online). 2017 ;835( 2): 236.[citado 2024 jun. 20 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
Artigo de periodico
Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars (2016)
Spina, Lorenzo; Moreno, Jorge Luiz Meléndez; Ramírez, Iván
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA
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ABNT
SPINA, Lorenzo e MORENO, Jorge Luiz Meléndez e RAMÍREZ, Iván. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, v. 585, p. A152/1-A152/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527429. Acesso em: 20 jun. 2024.
APA
Spina, L., Moreno, J. L. M., & Ramírez, I. (2016). Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars. Astronomy & Astrophysics, 585, A152/1-A152/15. doi:10.1051/0004-6361/201527429
NLM
Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527429
Vancouver
Spina L, Moreno JLM, Ramírez I. Planet signatures and effect of the chemical evolution of the Galactic thin-disk stars [Internet]. Astronomy & Astrophysics. 2016 ; 585 A152/1-A152/15.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527429
Artigo de periodico
Serendipitous discovery of the faint solar twin Inti 1 (2016)
Galarza, Jhon Yana; Moreno, Jorge Luiz Meléndez; Cohen, Judith G
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, TERRA (PLANETA), PLANETAS
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ABNT
GALARZA, Jhon Yana e MORENO, Jorge Luiz Meléndez e COHEN, Judith G. Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, v. 589, p. A65/1-A65/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527477. Acesso em: 20 jun. 2024.
APA
Galarza, J. Y., Moreno, J. L. M., & Cohen, J. G. (2016). Serendipitous discovery of the faint solar twin Inti 1. Astronomy & Astrophysics, 589, A65/1-A65/8. doi:10.1051/0004-6361/201527477
NLM
Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527477
Vancouver
Galarza JY, Moreno JLM, Cohen JG. Serendipitous discovery of the faint solar twin Inti 1 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A65/1-A65/8.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527477
Artigo de periodico
The Hyades open cluster is chemically inhomogeneous (2016)
Liu, F; Yong, D; Asplund, M; Ramírez, I; Moreno, Jorge Luiz Meléndez
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
LIU, F et al. The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, v. 457, p. 3934-3948, 2016Tradução . . Disponível em: https://doi.org/10.1093/mnras/stw247. Acesso em: 20 jun. 2024.
APA
Liu, F., Yong, D., Asplund, M., Ramírez, I., & Moreno, J. L. M. (2016). The Hyades open cluster is chemically inhomogeneous. Monthly Notices of the Royal Astronomical Society, 457, 3934-3948. doi:10.1093/mnras/stw247
NLM
Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1093/mnras/stw247
Vancouver
Liu F, Yong D, Asplund M, Ramírez I, Moreno JLM. The Hyades open cluster is chemically inhomogeneous [Internet]. Monthly Notices of the Royal Astronomical Society. 2016 ; 457 3934-3948.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1093/mnras/stw247
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: 20 jun. 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 jun. 20 ] 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 jun. 20 ] Available from: https://doi.org/10.1093/mnras/stv2821
Artigo de periodico
High-precision analysis of the solar twin HIP 100963 (2016)
Galarza, Jhon Yana; Moreno, Jorge Luiz Meléndez; Ramírez, Ivan; Yong, David; Karakas, Amanda I; Asplund, Martin; Liu, Fan
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, PLANETAS
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ABNT
GALARZA, Jhon Yana et al. High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, v. 589, p. A17/1-A17/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527912. Acesso em: 20 jun. 2024.
APA
Galarza, J. Y., Moreno, J. L. M., Ramírez, I., Yong, D., Karakas, A. I., Asplund, M., & Liu, F. (2016). High-precision analysis of the solar twin HIP 100963. Astronomy & Astrophysics, 589, A17/1-A17/8. doi:10.1051/0004-6361/201527912
NLM
Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527912
Vancouver
Galarza JY, Moreno JLM, Ramírez I, Yong D, Karakas AI, Asplund M, Liu F. High-precision analysis of the solar twin HIP 100963 [Internet]. Astronomy & Astrophysics. 2016 ; 589 A17/1-A17/8.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527912
Artigo de periodico
Correlation between lithium abundances and ages of solar twin stars (2016)
Carlos, Marília; Nissen, Poul E; Moreno, Jorge Luiz Meléndez
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, EVOLUÇÃO ESTELAR, PLANETAS
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ABNT
CARLOS, Marília e NISSEN, Poul E e MORENO, Jorge Luiz Meléndez. Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, v. 587, p. A100/1-A100/6, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527478. Acesso em: 20 jun. 2024.
APA
Carlos, M., Nissen, P. E., & Moreno, J. L. M. (2016). Correlation between lithium abundances and ages of solar twin stars. Astronomy & Astrophysics, 587, A100/1-A100/6. doi:10.1051/0004-6361/201527478
NLM
Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527478
Vancouver
Carlos M, Nissen PE, Moreno JLM. Correlation between lithium abundances and ages of solar twin stars [Internet]. Astronomy & Astrophysics. 2016 ; 587 A100/1-A100/6.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201527478
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: 20 jun. 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 jun. 20 ] 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 jun. 20 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
Artigo de periodico
Chemical signatures of planets: beyond solar-twins (2014)
Ramírez, I; Moreno, Jorge Luiz Meléndez; Asplund, M
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, PLANETAS
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ABNT
RAMÍREZ, I e MORENO, Jorge Luiz Meléndez e ASPLUND, M. Chemical signatures of planets: beyond solar-twins. Astronomy & Astrophysics, v. 561, p. A7/1-A7/16, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322558. Acesso em: 20 jun. 2024.
APA
Ramírez, I., Moreno, J. L. M., & Asplund, M. (2014). Chemical signatures of planets: beyond solar-twins. Astronomy & Astrophysics, 561, A7/1-A7/16. doi:10.1051/0004-6361/201322558
NLM
Ramírez I, Moreno JLM, Asplund M. Chemical signatures of planets: beyond solar-twins [Internet]. Astronomy & Astrophysics. 2014 ;561 A7/1-A7/16.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201322558
Vancouver
Ramírez I, Moreno JLM, Asplund M. Chemical signatures of planets: beyond solar-twins [Internet]. Astronomy & Astrophysics. 2014 ;561 A7/1-A7/16.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201322558
Artigo de periodico
HIP 114328: a new refractory-poor and Li-poor solar twin (2014)
Moreno, Jorge Luiz Meléndez; Schirbel, Lucas; Monroe, TalaWanda R; Yong, David; Ramírez, Iván; Asplund, Martin
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: SOL, ABUNDÂNCIAS SOLARES, ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS
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ABNT
MORENO, Jorge Luiz Meléndez et al. HIP 114328: a new refractory-poor and Li-poor solar twin. Astronomy & Astrophysics, v. 567, p. L3/1-L3/5, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424172. Acesso em: 20 jun. 2024.
APA
Moreno, J. L. M., Schirbel, L., Monroe, T. W. R., Yong, D., Ramírez, I., & Asplund, M. (2014). HIP 114328: a new refractory-poor and Li-poor solar twin. Astronomy & Astrophysics, 567, L3/1-L3/5. doi:10.1051/0004-6361/201424172
NLM
Moreno JLM, Schirbel L, Monroe TWR, Yong D, Ramírez I, Asplund M. HIP 114328: a new refractory-poor and Li-poor solar twin [Internet]. Astronomy & Astrophysics. 2014 ; 567 L3/1-L3/5.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201424172
Vancouver
Moreno JLM, Schirbel L, Monroe TWR, Yong D, Ramírez I, Asplund M. HIP 114328: a new refractory-poor and Li-poor solar twin [Internet]. Astronomy & Astrophysics. 2014 ; 567 L3/1-L3/5.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201424172
Artigo de periodico
A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation (2014)
Liu, F; Asplund, M; Ramírez, I; Yong, D; Moreno, Jorge Luiz Meléndez
Source: Monthly Notices of the Royal Astronomical Society Letters. Unidade: IAG
Subjects: PLANETAS, SATÉLITES, FORMAÇÃO DO SISTEMA SOLAR, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESTRELAS BINÁRIAS
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ABNT
LIU, F et al. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, v. 442, p. L51-L55, 2014Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slu055. Acesso em: 20 jun. 2024.
APA
Liu, F., Asplund, M., Ramírez, I., Yong, D., & Moreno, J. L. M. (2014). A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation. Monthly Notices of the Royal Astronomical Society Letters, 442, L51-L55. doi:10.1093/mnrasl/slu055
NLM
Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1093/mnrasl/slu055
Vancouver
Liu F, Asplund M, Ramírez I, Yong D, Moreno JLM. A high-precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation [Internet]. Monthly Notices of the Royal Astronomical Society Letters. 2014 ; 442 L51-L55.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1093/mnrasl/slu055
Artigo de periodico
High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun (2013)
Monroe, Tala Wanda R; Moreno, Jorge Luis Meléndez; Maia, Marcelo Tucci; Freitas, Fabrício C
Source: The Astrophysical Journal Letters. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS SOLARES
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ABNT
MONROE, Tala Wanda R et al. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun. The Astrophysical Journal Letters, v. 774, p. L32/1-L32/6, 2013Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/774/2/L32. Acesso em: 20 jun. 2024.
APA
Monroe, T. W. R., Moreno, J. L. M., Maia, M. T., & Freitas, F. C. (2013). High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun. The Astrophysical Journal Letters, 774, L32/1-L32/6. doi:10.1088/2041-8205/774/2/L32
NLM
Monroe TWR, Moreno JLM, Maia MT, Freitas FC. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun [Internet]. The Astrophysical Journal Letters. 2013 ; 774 L32/1-L32/6.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
Vancouver
Monroe TWR, Moreno JLM, Maia MT, Freitas FC. High precision abundances of the old solar twin HIP 102152: insights on Li depletion from the oldest Sun [Internet]. The Astrophysical Journal Letters. 2013 ; 774 L32/1-L32/6.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
Artigo de periodico
Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample (2012)
Santos, N. C; Lovis, C; Meléndez Moreno, Jorge Luis; Montalto, M; Naef, D; Pace, G
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: PLANETAS, ESTRELAS, ABUNDÂNCIA ESTELAR, ESPECTROSCOPIA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
SANTOS, N. C et al. Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample. Astronomy & Astrophysics, v. 538, p. A151/1-A151/6, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118276. Acesso em: 20 jun. 2024.
APA
Santos, N. C., Lovis, C., Meléndez Moreno, J. L., Montalto, M., Naef, D., & Pace, G. (2012). Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample. Astronomy & Astrophysics, 538, A151/1-A151/6. doi:10.1051/0004-6361/201118276
NLM
Santos NC, Lovis C, Meléndez Moreno JL, Montalto M, Naef D, Pace G. Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample [Internet]. Astronomy & Astrophysics. 2012 ; 538 A151/1-A151/6.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201118276
Vancouver
Santos NC, Lovis C, Meléndez Moreno JL, Montalto M, Naef D, Pace G. Metallicities for six nearby open clusters from high-resolution spectra of giant stars: [Fe/H] values for a planet search sample [Internet]. Astronomy & Astrophysics. 2012 ; 538 A151/1-A151/6.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1051/0004-6361/201118276
Artigo de periodico
Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? (2011)
Ramírez, I; Meléndez Moreno, Jorge Luis; Cornejo, D; Roederer, I. U; Fish, J. R
Source: The Astrophysical Journal. Unidade: IAG
Subjects: PLANETAS, ABUNDÂNCIA ESTELAR, ESTRELAS
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RAMÍREZ, I et al. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation?. The Astrophysical Journal, v. 740, p. 76/1-76/15, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/740/2/76. Acesso em: 20 jun. 2024.
APA
Ramírez, I., Meléndez Moreno, J. L., Cornejo, D., Roederer, I. U., & Fish, J. R. (2011). Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? The Astrophysical Journal, 740, 76/1-76/15. doi:10.1088/0004-637X/740/2/76
NLM
Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76
Vancouver
Ramírez I, Meléndez Moreno JL, Cornejo D, Roederer IU, Fish JR. Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation? [Internet]. The Astrophysical Journal. 2011 ; 740 76/1-76/15.[citado 2024 jun. 20 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76

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