Filtros : "ATMOSFERAS ESTELARES" "IAG-AGA" Removidos: "RADIOASTRONOMIA" "Alcaniz, J. S" "Hamaguchi, Kenji" 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: 18 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. 18 ] 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. 18 ] 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: 18 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. 18 ] 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. 18 ] 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: 18 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
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      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. 18 ] 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. 18 ] Available from: https://doi.org/10.3847/1538-4365/ab9c19
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES

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      OLIVEIRA, R. A. P. et al. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab6f76. Acesso em: 18 nov. 2024.
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      Oliveira, R. A. P., Souza, S. O., keber, L. O., & Barbuy, B. L. S. (2020). The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab6f76
    • NLM

      Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
    • Vancouver

      Oliveira RAP, Souza SO, keber LO, Barbuy BLS. The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XX. Ages of Single and Multiple Stellar Populations in Seven Bulge Globular Clusters [Internet]. The Astrophysical Journal. 2020 ; No( 1): 28/1-28/23.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab6f76
  • Source: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. Unidade: IAG

    Subjects: ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES

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      BARBOSA, Carlos Eduardo et al. One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v. 231, n. 1, p. 1, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/ab7660. Acesso em: 18 nov. 2024.
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      Barbosa, C. E., Oliveira, C. L. M. de, Molino, A., Costa-Duarte, M. V., Coelho, P. R. T., Cortesi, A., et al. (2020). One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 231( 1), 1. doi:10.3847/1538-4365/ab7660
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      Barbosa CE, Oliveira CLM de, Molino A, Costa-Duarte MV, Coelho PRT, Cortesi A, Herpich FR, Hernandez-Jimenez JA, Santos-Silva T, Pereira ES, Werle A, Overzier R, Ribeiro T. One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2020 ;231( 1): 1.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/ab7660
    • Vancouver

      Barbosa CE, Oliveira CLM de, Molino A, Costa-Duarte MV, Coelho PRT, Cortesi A, Herpich FR, Hernandez-Jimenez JA, Santos-Silva T, Pereira ES, Werle A, Overzier R, Ribeiro T. One hundred SMUDGes in S-PLUS: ultra-diffuse galaxies flourish in the field [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2020 ;231( 1): 1.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/ab7660
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: GALÁXIAS, ATMOSFERAS ESTELARES

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      COELHO, Paula Rodrigues Teixeira et al. To use or not to use synthetic stellar spectra in population synthesis models?. Monthly Notices of the Royal Astronomical Society, v. 491, n. 2, p. 2025-2042, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz3609. Acesso em: 18 nov. 2024.
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      Coelho, P. R. T., Bruzual, G., Gonçalves, T. S., & Charlot, S. (2020). To use or not to use synthetic stellar spectra in population synthesis models? Monthly Notices of the Royal Astronomical Society, 491( 2), 2025-2042. doi:10.1093/mnras/stz3609
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      Coelho PRT, Bruzual G, Gonçalves TS, Charlot S. To use or not to use synthetic stellar spectra in population synthesis models? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 2): 2025-2042.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz3609
    • Vancouver

      Coelho PRT, Bruzual G, Gonçalves TS, Charlot S. To use or not to use synthetic stellar spectra in population synthesis models? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 491( 2): 2025-2042.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1093/mnras/stz3609
  • 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: 18 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. 18 ] 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. 18 ] 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: 18 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. 18 ] 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. 18 ] 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: 18 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. 18 ] 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. 18 ] Available from: https://doi.org/10.1093/mnras/stz754
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: FOTOMETRIA, ATMOSFERAS ESTELARES

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      WHITTEN, D. D et al. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX. Astronomy & Astrophysics, v. 622, p. A182, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833368. Acesso em: 18 nov. 2024.
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      Whitten, D. D., Coelho, P. R. T., Costa-Duarte, M. V., Oliveira, C. L. M. de, Rossi, S. C. F., Sodré Júnior, L., & Hernandez-Jimenez, P. (2019). J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX. Astronomy & Astrophysics, 622, A182. doi:10.1051/0004-6361/201833368
    • NLM

      Whitten DD, Coelho PRT, Costa-Duarte MV, Oliveira CLM de, Rossi SCF, Sodré Júnior L, Hernandez-Jimenez P. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX [Internet]. Astronomy & Astrophysics. 2019 ; 622 A182.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201833368
    • Vancouver

      Whitten DD, Coelho PRT, Costa-Duarte MV, Oliveira CLM de, Rossi SCF, Sodré Júnior L, Hernandez-Jimenez P. J-PLUS: Identification of low-metallicity stars with artificial neural networks using SPHINX [Internet]. Astronomy & Astrophysics. 2019 ; 622 A182.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201833368
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES

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      MOURA, T. C et al. Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, v. No, n. 1, p. 28/1-28/23, 2019Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/ab3eb6. Acesso em: 18 nov. 2024.
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      Moura, T. C., Trevisan, M., Barbuy, B. L. S., & Rossi, S. C. F. (2019). Integrated Spectra of Milky Way Globular Clusters. The Astrophysical Journal, No( 1), 28/1-28/23. doi:10.3847/1538-4357/ab3eb6
    • NLM

      Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
    • Vancouver

      Moura TC, Trevisan M, Barbuy BLS, Rossi SCF. Integrated Spectra of Milky Way Globular Clusters [Internet]. The Astrophysical Journal. 2019 ; No( 1): 28/1-28/23.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/ab3eb6
  • 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: 18 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. 18 ] 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. 18 ] Available from: https://doi.org/10.1051/0004-6361/201833953
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      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: 18 nov. 2024.
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      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
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      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 nov. 18 ] 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 nov. 18 ] Available from: https://doi.org/10.3847/1538-4357/aad190
  • Source: Astronomical Journal. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, ESPECTROSCOPIA

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      PLACCO, Vinicius M et al. Spectroscopic validation of low-metallicity stars from RAVE. Astronomical Journal, v. 155, n. 6, p. 256, 2018Tradução . . Disponível em: https://doi.org/10.3847/1538-3881/aac20c. Acesso em: 18 nov. 2024.
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      Placco, V. M., Beers, J., Santucci, R. M., Chanamé, J., & Rossi, S. C. F. (2018). Spectroscopic validation of low-metallicity stars from RAVE. Astronomical Journal, 155( 6), 256. doi:10.3847/1538-3881/aac20c
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      Placco VM, Beers J, Santucci RM, Chanamé J, Rossi SCF. Spectroscopic validation of low-metallicity stars from RAVE [Internet]. Astronomical Journal. 2018 ; 155( 6): 256.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
    • Vancouver

      Placco VM, Beers J, Santucci RM, Chanamé J, Rossi SCF. Spectroscopic validation of low-metallicity stars from RAVE [Internet]. Astronomical Journal. 2018 ; 155( 6): 256.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-3881/aac20c
  • Source: Publications of the Astronomical Society of Australia. Unidade: IAG

    Assunto: ATMOSFERAS ESTELARES

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      BARBUY, Beatriz Leonor Silveira e TREVISAN, Julio e ALMEIDA, Amaury Augusto de. Calculation of molecular line intensity in stellar atmospheres. Publications of the Astronomical Society of Australia, v. 35, p. 1-11, 2018Tradução . . Disponível em: https://arxiv.org/pdf/1812.02414.pdf. Acesso em: 18 nov. 2024.
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      Barbuy, B. L. S., Trevisan, J., & Almeida, A. A. de. (2018). Calculation of molecular line intensity in stellar atmospheres. Publications of the Astronomical Society of Australia, 35, 1-11. doi:10.1017/pasa.2018.33
    • NLM

      Barbuy BLS, Trevisan J, Almeida AA de. Calculation of molecular line intensity in stellar atmospheres [Internet]. Publications of the Astronomical Society of Australia. 2018 ; 35 1-11.[citado 2024 nov. 18 ] Available from: https://arxiv.org/pdf/1812.02414.pdf
    • Vancouver

      Barbuy BLS, Trevisan J, Almeida AA de. Calculation of molecular line intensity in stellar atmospheres [Internet]. Publications of the Astronomical Society of Australia. 2018 ; 35 1-11.[citado 2024 nov. 18 ] Available from: https://arxiv.org/pdf/1812.02414.pdf
  • Source: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. Unidade: IAG

    Assunto: ATMOSFERAS ESTELARES

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      LEVENHAGEM, Ronaldo Savarino et al. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v. 231, n. 1, p. 1, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/aa7681. Acesso em: 18 nov. 2024.
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      Levenhagem, R. S., Diaz, M. P., Coelho, P. R. T., & Hubeny, I. (2017). A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 231( 1), 1. doi:10.3847/1538-4365/aa7681
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      Levenhagem RS, Diaz MP, Coelho PRT, Hubeny I. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2017 ;231( 1): 1.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/aa7681
    • Vancouver

      Levenhagem RS, Diaz MP, Coelho PRT, Hubeny I. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2017 ;231( 1): 1.[citado 2024 nov. 18 ] Available from: https://doi.org/10.3847/1538-4365/aa7681
  • Source: Canadian Journal of Physics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, EVOLUÇÃO ESTELAR

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      SANTRICH, Orlando J. Katime e ROSSI, Silvia Cristina Fernandes. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. Canadian Journal of Physics, v. 95, n. 9, p. 862-868, 2017Tradução . . Disponível em: https://doi.org/10.1139/cjp-2016-0912. Acesso em: 18 nov. 2024.
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      Santrich, O. J. K., & Rossi, S. C. F. (2017). High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725. Canadian Journal of Physics, 95( 9), 862-868. doi:10.1139/cjp-2016-0912
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      Santrich OJK, Rossi SCF. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725 [Internet]. Canadian Journal of Physics. 2017 ; 95( 9): 862-868.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1139/cjp-2016-0912
    • Vancouver

      Santrich OJK, Rossi SCF. High-resolution spectroscopy of giant stars in the open clusters IC 4651 and IC 4725 [Internet]. Canadian Journal of Physics. 2017 ; 95( 9): 862-868.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1139/cjp-2016-0912
  • Source: Astronomy and Astrophysysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, GALÁXIAS

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      FRIAÇA, Amâncio César Santos e BARBUY, Beatriz Leonor Silveira. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements*. Astronomy and Astrophysysics, v. 598, p. A121, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201629941. Acesso em: 18 nov. 2024.
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      Friaça, A. C. S., & Barbuy, B. L. S. (2017). Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements*. Astronomy and Astrophysysics, 598, A121. doi:10.1051/0004-6361/201629941
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      Friaça ACS, Barbuy BLS. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* [Internet]. Astronomy and Astrophysysics. 2017 ;598 A121.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201629941
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      Friaça ACS, Barbuy BLS. Tracing the evolution of the Galactic bulge with chemodynamical modelling of alpha-elements* [Internet]. Astronomy and Astrophysysics. 2017 ;598 A121.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201629941
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: PLANETAS, SATÉLITES, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      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: 18 nov. 2024.
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      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
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      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. 18 ] Available from: https://doi.org/10.1093/mnras/stw247
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      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. 18 ] Available from: https://doi.org/10.1093/mnras/stw247
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      VAN DER SWAELMEN, M et al. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, v. 586, p. A1/1-A1/11, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525709. Acesso em: 18 nov. 2024.
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      van der Swaelmen, M., Barbuy, B. L. S., Hill, V., Zoccali, M., Minniti, D., Ortolani, S., & Gómez, A. (2016). Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants. Astronomy & Astrophysics, 586, A1/1-A1/11. doi:10.1051/0004-6361/201525709
    • NLM

      van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201525709
    • Vancouver

      van der Swaelmen M, Barbuy BLS, Hill V, Zoccali M, Minniti D, Ortolani S, Gómez A. Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2016 ; 586 A1/1-A1/11.[citado 2024 nov. 18 ] Available from: https://doi.org/10.1051/0004-6361/201525709

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