Filtros : "ABUNDÂNCIA ESTELAR" "IAG" Removidos: "Indexado no: ProQuest" "European Southern Observatory" "Institut d'Astrophysique de Paris, Paris, France" "Berrocal Gomez, Jesus Antonio" "Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)" "Latin American Regional IAU Meeting" Limpar

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  • Source: Monthly Notices of the Royal Astronomical Society. Unidades: IAG, IF

    Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      RAZERA, R et al. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, v. 517, p. 4590-4606, 2022Tradução . . Disponível em: https://academic.oup.com/mnras/article/517/3/4590/6653110. Acesso em: 15 nov. 2024.
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      Razera, R., Barbuy, B. L. S., Moura, T. C., Ernandes, H., & Friaça, A. C. S. (2022). Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid. Monthly Notices of the Royal Astronomical Society, 517, 4590-4606. doi:10.1093/mnras/stac2136
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      Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2024 nov. 15 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
    • Vancouver

      Razera R, Barbuy BLS, Moura TC, Ernandes H, Friaça ACS. Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroid [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 517 4590-4606.[citado 2024 nov. 15 ] Available from: https://academic.oup.com/mnras/article/517/3/4590/6653110
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      ERNANDES, H et al. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, v. 510, p. 5362-5375, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3789. Acesso em: 15 nov. 2024.
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      Ernandes, H., Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Spite, M., Spite, F., et al. (2022). Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, 510, 5362-5375. doi:10.1093/mnras/stab3789
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      Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stab3789
    • Vancouver

      Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stab3789
  • Source: Astrophysical Journal Supplement Series. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      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: 15 nov. 2024.
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      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 nov. 15 ] 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 nov. 15 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      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: 15 nov. 2024.
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      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 nov. 15 ] 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 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab8bd7
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      NASCIMENTO J.-D. DO, et al. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, v. 898, p. 173 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab9c16. Acesso em: 15 nov. 2024.
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      Nascimento J.-D. do,, Almeida, L. de, Velloso, E. N., Anthony, F., Costa, J. S. da, Castro, M., & Moreno, J. L. M. (2020). Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2. Astrophysical Journal, 898, 173 2020. doi:10.3847/1538-4357/ab9c16
    • NLM

      Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
    • Vancouver

      Nascimento J.-D. do, Almeida L de, Velloso EN, Anthony F, Costa JS da, Castro M, Moreno JLM. Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2 [Internet]. Astrophysical Journal. 2020 ; 898 173 2020.[citado 2024 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab9c16
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      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: 15 nov. 2024.
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      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 nov. 15 ] 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 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad37d
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES

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      SOUZA, S. O et al. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster. The Astrophysical Journal, v. 890, p. 13 2020, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6a0f. Acesso em: 15 nov. 2024.
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      Souza, S. O., Kerber, L. de O., Barbuy, B. L. S., Pérez-Villegas, A., Oliveira, R. A. P., & Nardiello, D. (2020). Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster. The Astrophysical Journal, 890, 13 2020. doi:10.3847/1538-4357/ab6a0f
    • NLM

      Souza SO, Kerber L de O, Barbuy BLS, Pérez-Villegas A, Oliveira RAP, Nardiello D. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster [Internet]. The Astrophysical Journal. 2020 ; 890 13 2020.[citado 2024 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
    • Vancouver

      Souza SO, Kerber L de O, Barbuy BLS, Pérez-Villegas A, Oliveira RAP, Nardiello D. Self-consistent analysis of stellar clusters: an application to HST data of the halo globular cluster [Internet]. The Astrophysical Journal. 2020 ; 890 13 2020.[citado 2024 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/ab6a0f
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR

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      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: 15 nov. 2024.
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      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 nov. 15 ] 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 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/aad37d1a
  • Unidade: IAG

    Subjects: AGLOMERADOS DE GALÁXIAS, ESPECTROSCOPIA, ABUNDÂNCIA ESTELAR, ESTRELAS

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      REGGIANI, Henrique Marques. Abundâncias diferenciais em estrelas pobres em metais: impactos no estudo da Galáxia, evolução estelar nucleossíntese primordial. 2019. Tese (Doutorado) – Universidade de São Paulo, São Paulo, 2019. . Acesso em: 15 nov. 2024.
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      Reggiani, H. M. (2019). Abundâncias diferenciais em estrelas pobres em metais: impactos no estudo da Galáxia, evolução estelar nucleossíntese primordial (Tese (Doutorado). Universidade de São Paulo, São Paulo.
    • NLM

      Reggiani HM. Abundâncias diferenciais em estrelas pobres em metais: impactos no estudo da Galáxia, evolução estelar nucleossíntese primordial. 2019 ;[citado 2024 nov. 15 ]
    • Vancouver

      Reggiani HM. Abundâncias diferenciais em estrelas pobres em metais: impactos no estudo da Galáxia, evolução estelar nucleossíntese primordial. 2019 ;[citado 2024 nov. 15 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIA ESTELAR

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      FERNÁNDEZ-TRINCADO, D. G et al. H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia. Astronomy & Astrophysics, v. 627, p. A178, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834391. Acesso em: 15 nov. 2024.
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      Fernández-Trincado, D. G., Schiavon, R. P., Almeida, A. A. de, & Roman-Lopes, A. (2019). H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia. Astronomy & Astrophysics, 627, A178. doi:10.1051/0004-6361/201834391
    • NLM

      Fernández-Trincado DG, Schiavon RP, Almeida AA de, Roman-Lopes A. H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia [Internet]. Astronomy & Astrophysics. 2019 ; 627 A178.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201834391
    • Vancouver

      Fernández-Trincado DG, Schiavon RP, Almeida AA de, Roman-Lopes A. H-band discovery of additional second-generation stars in the Galactic bulge globular cluster NGC 6522 as observed by APOGEE and Gaia [Internet]. Astronomy & Astrophysics. 2019 ; 627 A178.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201834391
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESPECTROMETRIA, ATMOSFERAS ESTELARES

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      GALARZA, Jhon Yana et al. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, v. 490, p. L86-L90, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slz153. Acesso em: 15 nov. 2024.
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      Galarza, J. Y., Meléndez, J., Lorenzo-Oliveira, D., Reggiani, H., Carlos, M., & Ponte, G. (2019). The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515. Monthly Notices of the Royal Astronomical Society, 490, L86-L90. doi:10.1093/mnrasl/slz153
    • NLM

      Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnrasl/slz153
    • Vancouver

      Galarza JY, Meléndez J, Lorenzo-Oliveira D, Reggiani H, Carlos M, Ponte G. The effect stellar activity onthe spectroscopicstellar parameters of the young solar twin HIP 36515 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 490 L86-L90.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnrasl/slz153
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      PLACCO, Vinicius M e SANTUCCI, Rafael M e ROSSI, Silvia Cristina Fernandes. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, v. 870, n. 2, p. 122-1/122-11, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/aaf3b9. Acesso em: 15 nov. 2024.
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      Placco, V. M., Santucci, R. M., & Rossi, S. C. F. (2019). The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey. Astrophysical Journal, 870( 2), 122-1/122-11. doi:10.3847/1538-4357/aaf3b9
    • NLM

      Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2024 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
    • Vancouver

      Placco VM, Santucci RM, Rossi SCF. The R-Process Alliance: Spectroscopic Follow-up of Low-metallicity Star Candidates from the Best & Brightest Survey [Internet]. Astrophysical Journal. 2019 ; 870( 2): 122-1/122-11.[citado 2024 nov. 15 ] Available from: https://doi.org/10.3847/1538-4357/aaf3b9
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESPECTROSCOPIA

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      KNOWLES, Adam T et al. Stellar spectral models compared with empirical data. Monthly Notices of the Royal Astronomical Society, v. 486, n. 2, p. 1814-1832, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz754. Acesso em: 15 nov. 2024.
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      Knowles, A. T., Sansom, A. E., Coelho, P. R. T., Prieto, C. A., Conroy, C., & Vazdekis, A. (2019). Stellar spectral models compared with empirical data. Monthly Notices of the Royal Astronomical Society, 486( 2), 1814-1832. doi:10.1093/mnras/stz754
    • NLM

      Knowles AT, Sansom AE, Coelho PRT, Prieto CA, Conroy C, Vazdekis A. Stellar spectral models compared with empirical data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 2): 1814-1832.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stz754
    • Vancouver

      Knowles AT, Sansom AE, Coelho PRT, Prieto CA, Conroy C, Vazdekis A. Stellar spectral models compared with empirical data [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 486( 2): 1814-1832.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stz754
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ASTROQUÍMICA, ABUNDÂNCIA ESTELAR, JATOS (ASTRONOMIA)

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      DURONEA, N. U et al. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103. Monthly Notices of the Royal Astronomical Society, v. 489, n. 2, p. 1519-1532, 2019Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz2087. Acesso em: 15 nov. 2024.
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      Duronea, N. U., Bronfman, L., Mendoza, E., Merello, M., Finger, R., Reyes, N., et al. (2019). Cyanoacetylene in the outflow/hot molecular core G331.512-0.103. Monthly Notices of the Royal Astronomical Society, 489( 2), 1519-1532. doi:10.1093/mnras/stz2087
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      Duronea NU, Bronfman L, Mendoza E, Merello M, Finger R, Reyes N, Hervias-Caimapo C, Faure A, Cappa CE, Arnal EM, Lépine JRD, Kleiner I, Nyman L-A. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 1519-1532.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stz2087
    • Vancouver

      Duronea NU, Bronfman L, Mendoza E, Merello M, Finger R, Reyes N, Hervias-Caimapo C, Faure A, Cappa CE, Arnal EM, Lépine JRD, Kleiner I, Nyman L-A. Cyanoacetylene in the outflow/hot molecular core G331.512-0.103 [Internet]. Monthly Notices of the Royal Astronomical Society. 2019 ; 489( 2): 1519-1532.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stz2087
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS BINARIAS

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      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: 15 nov. 2024.
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      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
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      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 nov. 15 ] 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 nov. 15 ] Available from: https://academic.oup.com/mnras/article/490/2/2448/5583050
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES

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      LAGIOIA, E. P et al. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, v. 475, n. 3, p. 4088-4103, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty083. Acesso em: 15 nov. 2024.
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      Lagioia, E. P., Milone, A. P., Marino, A. F., Cassisi, S., Aparicio, A. J., Piotto, G., et al. (2018). The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations. Monthly Notices of the Royal Astronomical Society, 475( 3), 4088-4103. doi:10.1093/mnras/sty083
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      Lagioia EP, Milone AP, Marino AF, Cassisi S, Aparicio AJ, Piotto G, Anderson J, Barbuy BLS. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 4088-4103.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/sty083
    • Vancouver

      Lagioia EP, Milone AP, Marino AF, Cassisi S, Aparicio AJ, Piotto G, Anderson J, Barbuy BLS. The hubble space telescope UV legacy survey of galactic globular clusters: XII. The RGB bumps of multiple stellar populations [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 475( 3): 4088-4103.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/sty083
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)

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      SPINA, Lorenzo e MORENO, Jorge Luis Meléndez e ALVES-BRITO, Alan. The temporal evolution of neutron-capture elements in the Galactic discs. Monthly Notices of the Royal Astronomical Society, v. 474, n. 2, p. 2580-2593, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx2938. Acesso em: 15 nov. 2024.
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      Spina, L., Moreno, J. L. M., & Alves-Brito, A. (2018). The temporal evolution of neutron-capture elements in the Galactic discs. Monthly Notices of the Royal Astronomical Society, 474( 2), 2580-2593. doi:10.1093/mnras/stx2938
    • NLM

      Spina L, Moreno JLM, Alves-Brito A. The temporal evolution of neutron-capture elements in the Galactic discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 474( 2): 2580-2593.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stx2938
    • Vancouver

      Spina L, Moreno JLM, Alves-Brito A. The temporal evolution of neutron-capture elements in the Galactic discs [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 474( 2): 2580-2593.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1093/mnras/stx2938
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, CENTRO GALÁCTICO, AGLOMERADOS (GALÁXIA), GALÁXIA (VIA LÁCTEA)

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      BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558. Astronomy & Astrophysics, v. 619, p. A178, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833953. Acesso em: 15 nov. 2024.
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      Barbuy, B. L. S., Muniz, L., Ortolani, S., Ernandes, H., Dias, B., Saviane, I., et al. (2018). High-resolution abundance analysis of four red giants in the globular cluster NGC 6558. Astronomy & Astrophysics, 619, A178. doi:10.1051/0004-6361/201833953
    • NLM

      Barbuy BLS, Muniz L, Ortolani S, Ernandes H, Dias B, Saviane I, Kerber L, Bica E, Pérez-Villegas A, Rossi L, Held EV. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 [Internet]. Astronomy & Astrophysics. 2018 ; 619 A178.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201833953
    • Vancouver

      Barbuy BLS, Muniz L, Ortolani S, Ernandes H, Dias B, Saviane I, Kerber L, Bica E, Pérez-Villegas A, Rossi L, Held EV. High-resolution abundance analysis of four red giants in the globular cluster NGC 6558 [Internet]. Astronomy & Astrophysics. 2018 ; 619 A178.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201833953
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, AGLOMERADOS (GALÁXIA)

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      ERNANDES, H et al. Iron-peak elements Sc, V, Mn, Cu, and Zn in Galactic bulge globular clusters. Astronomy & Astrophysics, v. 616, p. A18, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731708. Acesso em: 15 nov. 2024.
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      Ernandes, H., Barbuy, B. L. S., Alves-Brito, A., Friaça, A. C. S., Siqueira-Mello, C., & Allen, D. M. (2018). Iron-peak elements Sc, V, Mn, Cu, and Zn in Galactic bulge globular clusters. Astronomy & Astrophysics, 616, A18. doi:10.1051/0004-6361/201731708
    • NLM

      Ernandes H, Barbuy BLS, Alves-Brito A, Friaça ACS, Siqueira-Mello C, Allen DM. Iron-peak elements Sc, V, Mn, Cu, and Zn in Galactic bulge globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 616 A18.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201731708
    • Vancouver

      Ernandes H, Barbuy BLS, Alves-Brito A, Friaça ACS, Siqueira-Mello C, Allen DM. Iron-peak elements Sc, V, Mn, Cu, and Zn in Galactic bulge globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 616 A18.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201731708
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: FORMAÇÃO DE ESTRELAS, ABUNDÂNCIA ESTELAR

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      LIU, F et al. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation. Astronomy & Astrophysics, v. 614, p. A138, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201832701. Acesso em: 15 nov. 2024.
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      Liu, F., Yong, D., Asplund, M., Feltzing, S., Mustill, A. J., Moreno, J. L. M., et al. (2018). Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation. Astronomy & Astrophysics, 614, A138. doi:10.1051/0004-6361/201832701
    • NLM

      Liu F, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM, Ramírez I, Lin J. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation [Internet]. Astronomy & Astrophysics. 2018 ; 614 A138.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201832701
    • Vancouver

      Liu F, Yong D, Asplund M, Feltzing S, Mustill AJ, Moreno JLM, Ramírez I, Lin J. Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation [Internet]. Astronomy & Astrophysics. 2018 ; 614 A138.[citado 2024 nov. 15 ] Available from: https://doi.org/10.1051/0004-6361/201832701

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