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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ESTATÍSTICA

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      GALARZA, Carlos Andres e EDEROCLITE, Alessandro e SODRÉ JÚNIOR, Laerte. J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline. Astronomy & Astrophysics, v. 657, p. A35, 2022Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/202142402. Acesso em: 16 nov. 2024.
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      Galarza, C. A., Ederoclite, A., & Sodré Júnior, L. (2022). J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline. Astronomy & Astrophysics, 657, A35. doi:10.1051/0004-6361/202142402
    • NLM

      Galarza CA, Ederoclite A, Sodré Júnior L. J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline [Internet]. Astronomy & Astrophysics. 2022 ; 657 A35.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202142402
    • Vancouver

      Galarza CA, Ederoclite A, Sodré Júnior L. J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline [Internet]. Astronomy & Astrophysics. 2022 ; 657 A35.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202142402
  • Source: Astronomy & Astrophysics. Unidades: IF, IAG

    Subjects: ASTROFÍSICA, GALÁXIAS, ESTRELAS, FOTOMETRIA, ESPECTROSCOPIA, ANÁLISE DE DADOS

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      LÓPEZ-SANJUAN, C et al. The miniJPAS survey: White dwarf science with 56 optical filters. Astronomy & Astrophysics, v. 665, 2022Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/202243584. Acesso em: 16 nov. 2024.
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      López-Sanjuan, C., Abramo, L. R. W., Sodré Júnior, L., & Oliveira, C. L. M. de. (2022). The miniJPAS survey: White dwarf science with 56 optical filters. Astronomy & Astrophysics, 665. doi:10.1051/0004-6361/202243584
    • NLM

      López-Sanjuan C, Abramo LRW, Sodré Júnior L, Oliveira CLM de. The miniJPAS survey: White dwarf science with 56 optical filters [Internet]. Astronomy & Astrophysics. 2022 ; 665[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202243584
    • Vancouver

      López-Sanjuan C, Abramo LRW, Sodré Júnior L, Oliveira CLM de. The miniJPAS survey: White dwarf science with 56 optical filters [Internet]. Astronomy & Astrophysics. 2022 ; 665[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202243584
  • Source: Astronomy & Astrophysics. Unidades: IF, IAG

    Subjects: ASTROFÍSICA, GALÁXIAS, ESTRELAS, FOTOMETRIA, ESPECTROSCOPIA, ANÁLISE DE DADOS

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      MARTÍNEZ-SOLAECHE, G. et al. The miniJPAS survey: Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field. Astronomy & Astrophysics, v. 661, p. 21, 2022Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/202142812. Acesso em: 16 nov. 2024.
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      Martínez-Solaeche, G., Abramo, L. R., Sodré Jr., L., Ederoclite, A., & Oliveira, C. M. de. (2022). The miniJPAS survey: Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field. Astronomy & Astrophysics, 661, 21. doi:10.1051/0004-6361/202142812
    • NLM

      Martínez-Solaeche G, Abramo LR, Sodré Jr. L, Ederoclite A, Oliveira CM de. The miniJPAS survey: Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field [Internet]. Astronomy & Astrophysics. 2022 ; 661 21.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202142812
    • Vancouver

      Martínez-Solaeche G, Abramo LR, Sodré Jr. L, Ederoclite A, Oliveira CM de. The miniJPAS survey: Identification and characterization of the emission line galaxies down to z < 0.35 in the AEGIS field [Internet]. Astronomy & Astrophysics. 2022 ; 661 21.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202142812
  • Source: Astronomy & Astrophysics. Unidades: IF, IAG

    Subjects: ESTRELAS, GALÁXIAS

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      DELGADO, R. M. González e ABRAMO, Luis Raul Weber. The miniJPAS survey: The role of group environment in quenching star formation. Astronomy & Astrophysics, v. 666, 2022Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/202244030. Acesso em: 16 nov. 2024.
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      Delgado, R. M. G., & Abramo, L. R. W. (2022). The miniJPAS survey: The role of group environment in quenching star formation. Astronomy & Astrophysics, 666. doi:10.1051/0004-6361/202244030
    • NLM

      Delgado RMG, Abramo LRW. The miniJPAS survey: The role of group environment in quenching star formation [Internet]. Astronomy & Astrophysics. 2022 ; 666[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202244030
    • Vancouver

      Delgado RMG, Abramo LRW. The miniJPAS survey: The role of group environment in quenching star formation [Internet]. Astronomy & Astrophysics. 2022 ; 666[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/202244030
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, POPULAÇÕES ESTELARES, ESTRELAS

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      HILKER, M et al. The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311. Astronomy & Astrophysics, v. 619, p. A70, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731737. Acesso em: 16 nov. 2024.
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      Hilker, M., Richtler, T., Barbosa, C. E., Arnaboldi, M., Coccato, L., & Oliveira, C. M. de. (2018). The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311. Astronomy & Astrophysics, 619, A70. doi:10.1051/0004-6361/201731737
    • NLM

      Hilker M, Richtler T, Barbosa CE, Arnaboldi M, Coccato L, Oliveira CM de. The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311 [Internet]. Astronomy & Astrophysics. 2018 ;619 A70.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201731737
    • Vancouver

      Hilker M, Richtler T, Barbosa CE, Arnaboldi M, Coccato L, Oliveira CM de. The Hydra I cluster core: II. Kinematic complexity in a rising velocity dispersion profile around the cD galaxy NGC 3311 [Internet]. Astronomy & Astrophysics. 2018 ;619 A70.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201731737
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, FOTOMETRIA

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      BAADE, Dietrich et al. Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★. Astronomy & Astrophysics, v. 610, n. A70 p. 17p, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201731187. Acesso em: 16 nov. 2024.
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      Baade, D., Pigulski, A., Rivinius, T., Carciofi, A. C., Panoglou, D., Ghoreyshi, M. R., et al. (2018). Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★. Astronomy & Astrophysics, 610( A70 p. 17p). doi:10.1051/0004-6361/201731187
    • NLM

      Baade D, Pigulski A, Rivinius T, Carciofi AC, Panoglou D, Ghoreyshi MR, Handler G, Kuschnig R, Moffat AFJ, Pablo H, Popowicz A, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★ [Internet]. Astronomy & Astrophysics. 2018 ; 610( A70 p. 17p):[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201731187
    • Vancouver

      Baade D, Pigulski A, Rivinius T, Carciofi AC, Panoglou D, Ghoreyshi MR, Handler G, Kuschnig R, Moffat AFJ, Pablo H, Popowicz A, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★ [Internet]. Astronomy & Astrophysics. 2018 ; 610( A70 p. 17p):[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201731187
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)

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      VÁSQUEZ, S et al. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters. Astronomy & Astrophysics, v. 619, p. A13, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201833525. Acesso em: 16 nov. 2024.
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      Vásquez, S., Saviane, I., Held, E. V., Da Costa, G. S., Dias, B., Gullieuszik, M., et al. (2018). Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters. Astronomy & Astrophysics, 619, A13. doi:10.1051/0004-6361/201833525
    • NLM

      Vásquez S, Saviane I, Held EV, Da Costa GS, Dias B, Gullieuszik M, Barbuy BLS, Ortolani S, Zoccali M. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 619 A13.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201833525
    • Vancouver

      Vásquez S, Saviane I, Held EV, Da Costa GS, Dias B, Gullieuszik M, Barbuy BLS, Ortolani S, Zoccali M. Homogeneous metallicities and radial velocities for Galactic globular clusters: II. New CaT metallicities for 28 distant and reddened globular clusters [Internet]. Astronomy & Astrophysics. 2018 ; 619 A13.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201833525
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, EVOLUÇÃO ESTELAR

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      BAZOT, M et al. Modelling the solar twin 18 Scorpii. Astronomy & Astrophysics, v. 619, p. A172, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834058. Acesso em: 16 nov. 2024.
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      Bazot, M., Creevey, O., Christensen-Dalsgaard, J., & Moreno, J. L. M. (2018). Modelling the solar twin 18 Scorpii. Astronomy & Astrophysics, 619, A172. doi:10.1051/0004-6361/201834058
    • NLM

      Bazot M, Creevey O, Christensen-Dalsgaard J, Moreno JLM. Modelling the solar twin 18 Scorpii [Internet]. Astronomy & Astrophysics. 2018 ; 619 A172.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201834058
    • Vancouver

      Bazot M, Creevey O, Christensen-Dalsgaard J, Moreno JLM. Modelling the solar twin 18 Scorpii [Internet]. Astronomy & Astrophysics. 2018 ; 619 A172.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201834058
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, FOTOMETRIA

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      BAADE, D et al. Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe). Astronomy & Astrophysics, v. 620, p. A145, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201834161. Acesso em: 16 nov. 2024.
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      Baade, D., Pigulski, A., Rivinius, T., Wang, L., Martayan, C., Handler, G., et al. (2018). Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe). Astronomy & Astrophysics, 620, A145. doi:10.1051/0004-6361/201834161
    • NLM

      Baade D, Pigulski A, Rivinius T, Wang L, Martayan C, Handler G, Panoglou D, Carciofi AC, Kuschnig R, Mehner A, Moffat AFJ, Pablo H, Rucinski SM, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe) [Internet]. Astronomy & Astrophysics. 2018 ; 620 A145.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201834161
    • Vancouver

      Baade D, Pigulski A, Rivinius T, Wang L, Martayan C, Handler G, Panoglou D, Carciofi AC, Kuschnig R, Mehner A, Moffat AFJ, Pablo H, Rucinski SM, Wade GA, Weiss WW, Zwintz K. Short-term variability and mass loss in Be stars: IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe) [Internet]. Astronomy & Astrophysics. 2018 ; 620 A145.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201834161
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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      KLEMENT, R et al. Multitechnique testing of the viscous decretion disk model - I. The stable and tenuous disk of the late-type Be star β CMi: (Corrigendum). Astronomy & Astrophysics, v. 607, p. C1, 2017Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526535e. Acesso em: 16 nov. 2024.
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      Klement, R., Carciofi, A. C., Rivinius, T., Panoglou, D., Vieira, R. G., & Faes, D. M. (2017). Multitechnique testing of the viscous decretion disk model - I. The stable and tenuous disk of the late-type Be star β CMi: (Corrigendum). Astronomy & Astrophysics, 607, C1. doi:10.1051/0004-6361/201526535e
    • NLM

      Klement R, Carciofi AC, Rivinius T, Panoglou D, Vieira RG, Faes DM. Multitechnique testing of the viscous decretion disk model - I. The stable and tenuous disk of the late-type Be star β CMi: (Corrigendum) [Internet]. Astronomy & Astrophysics. 2017 ; 607 C1.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201526535e
    • Vancouver

      Klement R, Carciofi AC, Rivinius T, Panoglou D, Vieira RG, Faes DM. Multitechnique testing of the viscous decretion disk model - I. The stable and tenuous disk of the late-type Be star β CMi: (Corrigendum) [Internet]. Astronomy & Astrophysics. 2017 ; 607 C1.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201526535e
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, PLANETAS, GALÁXIA (VIA LÁCTEA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      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: 16 nov. 2024.
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      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. 16 ] 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. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527429
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: SOL, ESTRELAS

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      SANTOS, Leonardo A. dos et al. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, v. 592, p. A156/1-A156/8, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628558. Acesso em: 16 nov. 2024.
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      Santos, L. A. dos, Moreno, J. L. M., Nascimento Júnior, J. D. do, Bedell, M., Ramírez, I., Bean, J. L., et al. (2016). The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars. Astronomy & Astrophysics, 592, A156/1-A156/8. doi:10.1051/0004-6361/201628558
    • NLM

      Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628558
    • Vancouver

      Santos LA dos, Moreno JLM, Nascimento Júnior JD do, Bedell M, Ramírez I, Bean JL, Asplund M, Spina L, Dreizler S, Brito AA, Casagrande L. The Solar Twin Planet Search: IV. The Sun as a typical rotator and evidence for a new rotational braking law for Sun-like stars [Internet]. Astronomy & Astrophysics. 2016 ; 592 A156/1-A156/8.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628558
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS, ESPECTROSCOPIA

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      THYGESEN, A. O et al. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, v. 588, p. A66, 2016Tradução . . Disponível em: https://arxiv.org/pdf/1602.00058.pdf. Acesso em: 16 nov. 2024.
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      Thygesen, A. O., Sbordone, L., Ludwig, H. -G., Ventura, P., Yong, D., Collet, R., et al. (2016). The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios. Astronomy & Astrophysics, 588, A66. doi:10.1051/0004-6361/201526643
    • NLM

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 nov. 16 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
    • Vancouver

      Thygesen AO, Sbordone L, Ludwig H-G, Ventura P, Yong D, Collet R, Christlieb N, Moreno JLM, Zaggia S. The chemical composition of red giants in 47 Tucanae: II. Magnesium isotopes and pollution scenarios [Internet]. Astronomy & Astrophysics. 2016 ; 588 A66.[citado 2024 nov. 16 ] Available from: https://arxiv.org/pdf/1602.00058.pdf
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, PERDA DE MASSA

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      BAADE, D et al. Short-term variability and mass loss in Be stars: I. BRITE satellite photometry of η and μ Centauri. Astronomy & Astrophysics, v. 588, p. A56/1-A56/18, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201528026. Acesso em: 16 nov. 2024.
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      Baade, D., Rivinius, T., Pigulski, A., Carciofi, A. C., Martayan, C., Moffat, A. F. J., et al. (2016). Short-term variability and mass loss in Be stars: I. BRITE satellite photometry of η and μ Centauri. Astronomy & Astrophysics, 588, A56/1-A56/18. doi:10.1051/0004-6361/201528026
    • NLM

      Baade D, Rivinius T, Pigulski A, Carciofi AC, Martayan C, Moffat AFJ, Wade GA, Weiss WW, Grunhut J, Handler G, Kuschnig R, Mehner A, Pablo H, Popowicz A, Rucinski S, Whittaker G. Short-term variability and mass loss in Be stars: I. BRITE satellite photometry of η and μ Centauri [Internet]. Astronomy & Astrophysics. 2016 ; 588 A56/1-A56/18.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201528026
    • Vancouver

      Baade D, Rivinius T, Pigulski A, Carciofi AC, Martayan C, Moffat AFJ, Wade GA, Weiss WW, Grunhut J, Handler G, Kuschnig R, Mehner A, Pablo H, Popowicz A, Rucinski S, Whittaker G. Short-term variability and mass loss in Be stars: I. BRITE satellite photometry of η and μ Centauri [Internet]. Astronomy & Astrophysics. 2016 ; 588 A56/1-A56/18.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201528026
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS

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      MORENO, Jorge Luiz Meléndez et al. 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star. Astronomy & Astrophysics, v. 585, p. L5/1-L5/5, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527456. Acesso em: 16 nov. 2024.
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      Moreno, J. L. M., Placco, V. M., Tucci-Maia, M., Ramírez, I., Li, T. S., & Perez, G. (2016). 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star. Astronomy & Astrophysics, 585, L5/1-L5/5. doi:10.1051/0004-6361/201527456
    • NLM

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star [Internet]. Astronomy & Astrophysics. 2016 ; 585 L5/1-L5/5.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527456
    • Vancouver

      Moreno JLM, Placco VM, Tucci-Maia M, Ramírez I, Li TS, Perez G. 2MASS J18082002-5104378: the brightest (V=11.9) ultra-metal poor star [Internet]. Astronomy & Astrophysics. 2016 ; 585 L5/1-L5/5.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527456
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), ESTRELAS

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      SPINA, L. et al. Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy. Astronomy & Astrophysics, v. 59, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628557. Acesso em: 16 nov. 2024.
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      Spina, L., Moreno, J. L. M., Karakas, A. I., Ramírez, I., Monroe, T. R., Asplund, M., & Yong, D. (2016). Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy. Astronomy & Astrophysics, 59. doi:10.1051/0004-6361/201628557
    • NLM

      Spina L, Moreno JLM, Karakas AI, Ramírez I, Monroe TR, Asplund M, Yong D. Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy [Internet]. Astronomy & Astrophysics. 2016 ; 59[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628557
    • Vancouver

      Spina L, Moreno JLM, Karakas AI, Ramírez I, Monroe TR, Asplund M, Yong D. Nucleosynthetic history of elements in the Galactic disk. [X/Fe]-age relations from high-precision spectroscopy [Internet]. Astronomy & Astrophysics. 2016 ; 59[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628557
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, POPULAÇÕES ESTELARES, ESTRELAS

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      BARBOSA, C. E et al. The Hydra I cluster core: I. Stellar populations in the cD galaxy NGC 3311. Astronomy & Astrophysics, v. 589, p. A139/1-A139/16, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628137. Acesso em: 16 nov. 2024.
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      Barbosa, C. E., Arnaboldi, M., Coccato, L., Hilker, M., Oliveira, C. L. M. de, & Richtler, T. (2016). The Hydra I cluster core: I. Stellar populations in the cD galaxy NGC 3311. Astronomy & Astrophysics, 589, A139/1-A139/16. doi:10.1051/0004-6361/201628137
    • NLM

      Barbosa CE, Arnaboldi M, Coccato L, Hilker M, Oliveira CLM de, Richtler T. The Hydra I cluster core: I. Stellar populations in the cD galaxy NGC 3311 [Internet]. Astronomy & Astrophysics. 2016 ;589 A139/1-A139/16.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628137
    • Vancouver

      Barbosa CE, Arnaboldi M, Coccato L, Hilker M, Oliveira CLM de, Richtler T. The Hydra I cluster core: I. Stellar populations in the cD galaxy NGC 3311 [Internet]. Astronomy & Astrophysics. 2016 ;589 A139/1-A139/16.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201628137
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS, NUVENS DE MAGALHÃES

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      DIAS, B et al. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, v. 591, p. A11/1-A11/16, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527558. Acesso em: 16 nov. 2024.
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      Dias, B., Kerber, L., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2016). SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients. Astronomy & Astrophysics, 591, A11/1-A11/16. doi:10.1051/0004-6361/201527558
    • NLM

      Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ; 591 A11/1-A11/16.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527558
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Bica E, Ortolani S. SMC west halo: a slice of the galaxy that is being tidally stripped? Star clusters trace age and metallicity gradients [Internet]. Astronomy & Astrophysics. 2016 ; 591 A11/1-A11/16.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • Source: Meeting Abstracts. Conference titles: IAU General Assembly. Unidade: IAG

    Subjects: SOL, ESTRELAS, DÍNAMOS

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      KOSOVICHEV, Alexander et al. Effects of tachocline in solar-stellar dynamo simulations. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 16 nov. 2024.
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      Kosovichev, A., Guerrero, G., Smolarkiewicz, P., Dal Pino, E. M. de G., & Mansour, N. N. (2015). Effects of tachocline in solar-stellar dynamo simulations. In Meeting Abstracts. Paris: International Astronomical Union.
    • NLM

      Kosovichev A, Guerrero G, Smolarkiewicz P, Dal Pino EM de G, Mansour NN. Effects of tachocline in solar-stellar dynamo simulations. Meeting Abstracts. 2015 ;[citado 2024 nov. 16 ]
    • Vancouver

      Kosovichev A, Guerrero G, Smolarkiewicz P, Dal Pino EM de G, Mansour NN. Effects of tachocline in solar-stellar dynamo simulations. Meeting Abstracts. 2015 ;[citado 2024 nov. 16 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, CINEMÁTICA, DINÂMICA, POPULAÇÕES ESTELARES, GALÁXIA (VIA LÁCTEA)

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      DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, v. 573, p. A13/1-A13/23, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423996. Acesso em: 16 nov. 2024.
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      Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Costa, G. S. da, Ortolani, S., et al. (2015). FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8. Astronomy & Astrophysics, 573, A13/1-A13/23. doi:10.1051/0004-6361/201423996
    • NLM

      Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201423996
    • Vancouver

      Dias B, Barbuy BLS, Saviane I, Held EV, Costa GS da, Ortolani S, Vásquez S, Gullieuszik M, Katz D. FORS2/VLT survey of Milky Way globular clusters: I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8 [Internet]. Astronomy & Astrophysics. 2015 ; 573 A13/1-A13/23.[citado 2024 nov. 16 ] Available from: https://doi.org/10.1051/0004-6361/201423996

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