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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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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
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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] Available from: https://doi.org/10.1051/0004-6361/201527478

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