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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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] Available from: https://doi.org/10.3847/1538-4357/835/2/236
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
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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: 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
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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] Available from: https://doi.org/10.1088/0004-637X/808/1/13
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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] 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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] Available from: https://doi.org/10.1088/2041-8205/774/2/L32
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
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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: 03 nov. 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 nov. 03 ] 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 nov. 03 ] Available from: https://doi.org/10.1088/0004-637X/740/2/76

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