ReP USP - Resultado da busca

Artigo de periodico
Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger Observatory (2023)
Halim, Adila Binti Abdul ; Catalani, Fernando ; Souza, Vitor de ; Oliveira, Cainã de ; Armand, Johnnier Perez; Santos, Edivaldo Moura; Peixoto, Carlos Jose Todero
Source: Astrophysical Journal. Unidades: IFSC, EEL, IF
Subjects: RAIOS CÓSMICOS, FÍSICA DE ALTA ENERGIA, TELESCÓPIOS, ASTROFÍSICA
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ABNT
HALIM, Adila Binti Abdul et al. Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger Observatory. Astrophysical Journal, v. 952, n. 1, 2023Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/acc862. Acesso em: 25 jul. 2024.
APA
Halim, A. B. A., Catalani, F., Souza, V. de, Oliveira, C. de, Armand, J. P., Santos, E. M., & Peixoto, C. J. T. (2023). Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger Observatory. Astrophysical Journal, 952( 1). doi:10.3847/1538-4357/acc862
NLM
Halim ABA, Catalani F, Souza V de, Oliveira C de, Armand JP, Santos EM, Peixoto CJT. Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger Observatory [Internet]. Astrophysical Journal. 2023 ; 952( 1):[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/acc862
Vancouver
Halim ABA, Catalani F, Souza V de, Oliveira C de, Armand JP, Santos EM, Peixoto CJT. Search for ultra-high-energy photons from gravitational wave sources with the Pierre Auger Observatory [Internet]. Astrophysical Journal. 2023 ; 952( 1):[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/acc862
Artigo de periodico
How Magnetic Activity Alters What We Learn from Stellar Spectra (2020)
Spina, Lorenzo ; Moreno, Jorge Luis Meléndez ; Galarza, Jhon J. Yana
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e GALARZA, Jhon J. Yana. How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab8bd7. Acesso em: 25 jul. 2024.
APA
Spina, L., Moreno, J. L. M., & Galarza, J. J. Y. (2020). How Magnetic Activity Alters What We Learn from Stellar Spectra. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/ab8bd7
NLM
Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Vancouver
Spina L, Moreno JLM, Galarza JJY. How Magnetic Activity Alters What We Learn from Stellar Spectra [Internet]. Astrophysical Journal. 2020 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
Artigo de periodico
Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres (2018)
Spina, Lorenzo; Moreno, Jorge Luis Meléndez; Casey, Andrew R; Karakas, Amanda I; Tucci-Maia, Marcelo
Source: Astrophysical Journal. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES
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ABNT
SPINA, Lorenzo et al. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, v. 863, n. 2, p. 179-1/179-6, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aad190. Acesso em: 25 jul. 2024.
APA
Spina, L., Moreno, J. L. M., Casey, A. R., Karakas, A. I., & Tucci-Maia, M. (2018). Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres. Astrophysical Journal, 863( 2), 179-1/179-6. doi:10.3847/1538-4357/aad190
NLM
Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad190
Vancouver
Spina L, Moreno JLM, Casey AR, Karakas AI, Tucci-Maia M. Chemical inhomogeneities in the pleiades: signatures of rocky-forming material in stellar atmospheres [Internet]. Astrophysical Journal. 2018 ; 863( 2): 179-1/179-6.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad190
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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad908
Artigo de periodico
A formation timescale of the galactic Halo from Mg isotopes in dwarf stars (2018)
Carlos, Marília; Karakas, Amanda I; Cohen, Judith G; Kobayashi, Chiaki; Moreno, Jorge Luis Meléndez
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR
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ABNT
CARLOS, Marília et al. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, v. 856, n. 2, p. 161-1/161-7, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aab36c. Acesso em: 25 jul. 2024.
APA
Carlos, M., Karakas, A. I., Cohen, J. G., Kobayashi, C., & Moreno, J. L. M. (2018). A formation timescale of the galactic Halo from Mg isotopes in dwarf stars. Astrophysical Journal, 856( 2), 161-1/161-7. doi:10.3847/1538-4357/aab36c
NLM
Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
Vancouver
Carlos M, Karakas AI, Cohen JG, Kobayashi C, Moreno JLM. A formation timescale of the galactic Halo from Mg isotopes in dwarf stars [Internet]. Astrophysical Journal. 2018 ; 856( 2): 161-1/161-7.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aab36c
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
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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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
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: 25 jul. 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 jul. 25 ] 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 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/aa6a1d
Artigo de periodico
Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis (2017)
Beers, Timothy C; Placco, Vinicius M; Carollo, Daniela; Rossi, Silvia Cristina Fernandes; Lee, Young Sun; Frebel, Anna; Norris, John E; Dietz, Sarah; Masseron, Thomas
Source: Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR
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ABNT
BEERS, Timothy C et al. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis. Astrophysical Journal, v. 835, n. 1, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 25 jul. 2024.
APA
Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis. Astrophysical Journal, 835( 1), 81. doi:10.3847/1538-4357/835/1/81
NLM
Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis [Internet]. Astrophysical Journal. 2017 ;835( 1): 81.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
Vancouver
Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis [Internet]. Astrophysical Journal. 2017 ;835( 1): 81.[citado 2024 jul. 25 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81

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