Filtros : "Ortolani, S" "França" Limpar

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  • Source: Astronomy & Astrophysics. Unidade: IAG

    Assunto: GALÁXIA (VIA LÁCTEA)

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      ORTOLANI, S e BARBUY, Beatriz Leonor Silveira. Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆. Astronomy & Astrophysics, v. 627, p. A145, 2019Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201935726. Acesso em: 28 ago. 2024.
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      Ortolani, S., & Barbuy, B. L. S. (2019). Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆. Astronomy & Astrophysics, 627, A145. doi:10.1051/0004-6361/201935726
    • NLM

      Ortolani S, Barbuy BLS. Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆ [Internet]. Astronomy & Astrophysics. 2019 ; 627 A145.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201935726
    • Vancouver

      Ortolani S, Barbuy BLS. Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski 2)⋆ [Internet]. Astronomy & Astrophysics. 2019 ; 627 A145.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201935726
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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    • ABNT

      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: 28 ago. 2024.
    • APA

      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 ago. 28 ] 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 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201833953
  • 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: 28 ago. 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 ago. 28 ] 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 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201833525
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS

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      SILVEIRA, C. R. da et al. Oxygen and zinc abundances in 417 Galactic bulge red giants★. Astronomy & Astrophysics, v. 614, p. A149, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730562. Acesso em: 28 ago. 2024.
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      Silveira, C. R. da, Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Zoccali, M., Rafelski, S., et al. (2018). Oxygen and zinc abundances in 417 Galactic bulge red giants★. Astronomy & Astrophysics, 614, A149. doi:10.1051/0004-6361/201730562
    • NLM

      Silveira CR da, Barbuy BLS, Friaça ACS, Hill V, Zoccali M, Rafelski S, González OA, Minniti D, Renzini A, Ortolani S. Oxygen and zinc abundances in 417 Galactic bulge red giants★ [Internet]. Astronomy & Astrophysics. 2018 ; 614 A149.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201730562
    • Vancouver

      Silveira CR da, Barbuy BLS, Friaça ACS, Hill V, Zoccali M, Rafelski S, González OA, Minniti D, Renzini A, Ortolani S. Oxygen and zinc abundances in 417 Galactic bulge red giants★ [Internet]. Astronomy & Astrophysics. 2018 ; 614 A149.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201730562
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, DINÂMICA, CINEMÁTICA, POPULAÇÕES ESTELARES, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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      DIAS, B et al. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, v. 590, p. A9/1-A9/15, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526765. Acesso em: 28 ago. 2024.
    • APA

      Dias, B., Barbuy, B. L. S., Saviane, I., Held, E. V., Da Costa, G. S., Ortolani, S., et al. (2016). FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale. Astronomy & Astrophysics, 590, A9/1-A9/15. doi:10.1051/0004-6361/201526765
    • NLM

      Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201526765
    • Vancouver

      Dias B, Barbuy BLS, Saviane I, Held EV, Da Costa GS, Ortolani S, Gullieuszik M, Vásquez S. FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale [Internet]. Astronomy & Astrophysics. 2016 ; 590 A9/1-A9/15.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201526765
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, 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, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201527558. Acesso em: 28 ago. 2024.
    • APA

      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. 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 ;[citado 2024 ago. 28 ] 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 ;[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • 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: 28 ago. 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 ago. 28 ] 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 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201525709
  • 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: 28 ago. 2024.
    • APA

      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 ago. 28 ] 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 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • 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: 28 ago. 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 ago. 28 ] 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 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201423996
  • Source: Astronomy & Astrophysics. Unidades: IAG, FO

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA), GALÁXIAS (EVOLUÇÃO)

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      BARBUY, Beatriz Leonor Silveira et al. Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems. Astronomy & Astrophysics, v. 580, p. A40/1-A40/16, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201525694. Acesso em: 28 ago. 2024.
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      Barbuy, B. L. S., Friaça, A. C. S., Silveira, C. R. da, Hill, V., Zoccali, M., Minniti, D., et al. (2015). Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems. Astronomy & Astrophysics, 580, A40/1-A40/16. doi:10.1051/0004-6361/201525694
    • NLM

      Barbuy BLS, Friaça ACS, Silveira CR da, Hill V, Zoccali M, Minniti D, Renzini A, Ortolani S, Gómez A. Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems [Internet]. Astronomy & Astrophysics. 2015 ; 580 A40/1-A40/16.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201525694
    • Vancouver

      Barbuy BLS, Friaça ACS, Silveira CR da, Hill V, Zoccali M, Minniti D, Renzini A, Ortolani S, Gómez A. Zinc abundances in Galactic bulge field red giants: implications for damped Lyman-alpha systems [Internet]. Astronomy & Astrophysics. 2015 ; 580 A40/1-A40/16.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201525694
  • 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 red giants in the globular cluster NGC 6522. Astronomy & Astrophysics, v. 570, p. A76/1-A76/21, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424311. Acesso em: 28 ago. 2024.
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      Barbuy, B. L. S., Chiappini, C., Cantelli, E., Depagne, E., Pignatari, M., Hirschi, R., et al. (2014). High-resolution abundance analysis of red giants in the globular cluster NGC 6522. Astronomy & Astrophysics, 570, A76/1-A76/21. doi:10.1051/0004-6361/201424311
    • NLM

      Barbuy BLS, Chiappini C, Cantelli E, Depagne E, Pignatari M, Hirschi R, Cescutti G, Ortolani S, Hill V, Zoccali M, Minniti D, Trevisan M, Bica E, Gómez A. High-resolution abundance analysis of red giants in the globular cluster NGC 6522 [Internet]. Astronomy & Astrophysics. 2014 ; 570 A76/1-A76/21.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201424311
    • Vancouver

      Barbuy BLS, Chiappini C, Cantelli E, Depagne E, Pignatari M, Hirschi R, Cescutti G, Ortolani S, Hill V, Zoccali M, Minniti D, Trevisan M, Bica E, Gómez A. High-resolution abundance analysis of red giants in the globular cluster NGC 6522 [Internet]. Astronomy & Astrophysics. 2014 ; 570 A76/1-A76/21.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201424311
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS, NUVENS DE MAGALHÃES

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      DIAS, B. et al. Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling. Astronomy & Astrophysics, v. 561, p. A106/1-A106/14, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322092. Acesso em: 28 ago. 2024.
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      Dias, B., Kerber, L. O., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2014). Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling. Astronomy & Astrophysics, 561, A106/1-A106/14. doi:10.1051/0004-6361/201322092
    • NLM

      Dias B, Kerber LO, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling [Internet]. Astronomy & Astrophysics. 2014 ; 561 A106/1-A106/14.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201322092
    • Vancouver

      Dias B, Kerber LO, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling [Internet]. Astronomy & Astrophysics. 2014 ; 561 A106/1-A106/14.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201322092
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      BARBUY, Beatriz Leonor Silveira et al. Manganese abundances in Galactic bulge red giants. Astronomy & Astrophysics, v. 559, p. A5/1-A5/14, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322380. Acesso em: 28 ago. 2024.
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      Barbuy, B. L. S., Hill, V., Zocalli, M., Minniti, D., Renzini, A., Ortolani, S., et al. (2013). Manganese abundances in Galactic bulge red giants. Astronomy & Astrophysics, 559, A5/1-A5/14. doi:10.1051/0004-6361/201322380
    • NLM

      Barbuy BLS, Hill V, Zocalli M, Minniti D, Renzini A, Ortolani S, Gómez A, Trevisan M, Dutra N. Manganese abundances in Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2013 ; 559 A5/1-A5/14.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201322380
    • Vancouver

      Barbuy BLS, Hill V, Zocalli M, Minniti D, Renzini A, Ortolani S, Gómez A, Trevisan M, Dutra N. Manganese abundances in Galactic bulge red giants [Internet]. Astronomy & Astrophysics. 2013 ; 559 A5/1-A5/14.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201322380
  • Source: LARIM 2013: Abstract Book. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG

    Subjects: ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA), ZINCO

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      SILVEIRA, C. R et al. Abundânciasde zinco em estrelas do bojo Galáctico. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 28 ago. 2024.
    • APA

      Silveira, C. R., Barbuy, B. L. S., Hill, V., Zoccali, M., Minniti, D., Renzini, A., et al. (2013). Abundânciasde zinco em estrelas do bojo Galáctico. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
    • NLM

      Silveira CR, Barbuy BLS, Hill V, Zoccali M, Minniti D, Renzini A, Ortolani S, Gómez A, Dutra N. Abundânciasde zinco em estrelas do bojo Galáctico. LARIM 2013: Abstract Book. 2013 ;[citado 2024 ago. 28 ]
    • Vancouver

      Silveira CR, Barbuy BLS, Hill V, Zoccali M, Minniti D, Renzini A, Ortolani S, Gómez A, Dutra N. Abundânciasde zinco em estrelas do bojo Galáctico. LARIM 2013: Abstract Book. 2013 ;[citado 2024 ago. 28 ]
  • Source: LARIM 2013: Abstract Book. Conference titles: Latin American Regional IAU Meeting. Unidade: IAG

    Subjects: NUVENS DE MAGALHÃES, ESTRELAS

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      DIAS, B et al. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. 2013, Anais.. Paris: International Astronomical Union, 2013. . Acesso em: 28 ago. 2024.
    • APA

      Dias, B., Kerber, L., Barbuy, B. L. S., Santiago, B., Ortolani, S., & Balbinot, E. (2013). Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. In LARIM 2013: Abstract Book. Paris: International Astronomical Union.
    • NLM

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. LARIM 2013: Abstract Book. 2013 ;[citado 2024 ago. 28 ]
    • Vancouver

      Dias B, Kerber L, Barbuy BLS, Santiago B, Ortolani S, Balbinot E. Self-consistent physical parameters for 5 intermediate-age SMC stellar clusters from CMD modelling. LARIM 2013: Abstract Book. 2013 ;[citado 2024 ago. 28 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), GALÁXIAS

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      BARBUY, Beatriz Leonor Silveira et al. Deep imaging of Virgo Z: not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies (Research Note). Astronomy & Astrophysics, v. 559, p. A61/1-A61/4, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201321943. Acesso em: 28 ago. 2024.
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      Barbuy, B. L. S., Bica, E., Ortolani, S., & Lopes-Souza, A. (2013). Deep imaging of Virgo Z: not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies (Research Note). Astronomy & Astrophysics, 559, A61/1-A61/4. doi:10.1051/0004-6361/201321943
    • NLM

      Barbuy BLS, Bica E, Ortolani S, Lopes-Souza A. Deep imaging of Virgo Z: not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies (Research Note) [Internet]. Astronomy & Astrophysics. 2013 ; 559 A61/1-A61/4.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201321943
    • Vancouver

      Barbuy BLS, Bica E, Ortolani S, Lopes-Souza A. Deep imaging of Virgo Z: not a nearby ultrafaint dwarf galaxy, but a distant compact group of galaxies (Research Note) [Internet]. Astronomy & Astrophysics. 2013 ; 559 A61/1-A61/4.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201321943
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

    Acesso à fonteDOIHow to cite
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    • ABNT

      SAVIANE, I et al. Homogeneous metallicities and radial velocities for Galactic globular clusters: first CaT metallicities for twenty clusters. Astronomy & Astrophysics, v. 540, p. A27/1-A27/20, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201118138. Acesso em: 28 ago. 2024.
    • APA

      Saviane, I., Costa, G. S. da, Held, E. V., Sommariva, V., Gullieuszik, M., Barbuy, B. L. S., & Ortolani, S. (2012). Homogeneous metallicities and radial velocities for Galactic globular clusters: first CaT metallicities for twenty clusters. Astronomy & Astrophysics, 540, A27/1-A27/20. doi:10.1051/0004-6361/201118138
    • NLM

      Saviane I, Costa GS da, Held EV, Sommariva V, Gullieuszik M, Barbuy BLS, Ortolani S. Homogeneous metallicities and radial velocities for Galactic globular clusters: first CaT metallicities for twenty clusters [Internet]. Astronomy & Astrophysics. 2012 ; 540 A27/1-A27/20.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201118138
    • Vancouver

      Saviane I, Costa GS da, Held EV, Sommariva V, Gullieuszik M, Barbuy BLS, Ortolani S. Homogeneous metallicities and radial velocities for Galactic globular clusters: first CaT metallicities for twenty clusters [Internet]. Astronomy & Astrophysics. 2012 ; 540 A27/1-A27/20.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201118138
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA, GALÁXIAS, ESTRELAS

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      HILL, V et al. The metallicity distribution of bulge clump giants in Baade’s window. Astronomy & Astrophysics, v. 534, p. A80/1-A80/20, 2011Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/200913757. Acesso em: 28 ago. 2024.
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      Hill, V., Lecureur, A., Gómez, A., Zoccali, M., Schultheis, M., Babusiaux, C., et al. (2011). The metallicity distribution of bulge clump giants in Baade’s window. Astronomy & Astrophysics, 534, A80/1-A80/20. doi:10.1051/0004-6361/200913757
    • NLM

      Hill V, Lecureur A, Gómez A, Zoccali M, Schultheis M, Babusiaux C, Royer F, Barbuy BLS, Arenou F, Minniti D, Ortolani S. The metallicity distribution of bulge clump giants in Baade’s window [Internet]. Astronomy & Astrophysics. 2011 ; 534 A80/1-A80/20.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/200913757
    • Vancouver

      Hill V, Lecureur A, Gómez A, Zoccali M, Schultheis M, Babusiaux C, Royer F, Barbuy BLS, Arenou F, Minniti D, Ortolani S. The metallicity distribution of bulge clump giants in Baade’s window [Internet]. Astronomy & Astrophysics. 2011 ; 534 A80/1-A80/20.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/200913757
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), FORMAÇÃO E EVOLUÇÃO DA GALÁXIA

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    • ABNT

      GONZÁLEZ, O. A et al. Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants. Astronomy & Astrophysics, v. 530, p. A54/1-A54/12, 2011Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201116548. Acesso em: 28 ago. 2024.
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      González, O. A., Rejkuba, M., Zoccali, M., Hill, V., Battaglia, G., Babusiaux, C., et al. (2011). Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants. Astronomy & Astrophysics, 530, A54/1-A54/12. doi:10.1051/0004-6361/201116548
    • NLM

      González OA, Rejkuba M, Zoccali M, Hill V, Battaglia G, Babusiaux C, Minniti D, Barbuy BLS, Alves-Brito A, Renzini A, Gomez A, Ortolani S. Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants [Internet]. Astronomy & Astrophysics. 2011 ; 530 A54/1-A54/12.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201116548
    • Vancouver

      González OA, Rejkuba M, Zoccali M, Hill V, Battaglia G, Babusiaux C, Minniti D, Barbuy BLS, Alves-Brito A, Renzini A, Gomez A, Ortolani S. Alpha element abundances and gradients in the Milky Way bulge from FLAMES-GIRAFFE spectra of 650 K giants [Internet]. Astronomy & Astrophysics. 2011 ; 530 A54/1-A54/12.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/201116548
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS, INFRAVERMELHO, CENTRO GALÁCTICO, GALÁXIA (VIA LÁCTEA)

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    • ABNT

      RYDE, N et al. Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra. Astronomy & Astrophysics, v. 509, p. A20/1-A20/15, 2010Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/200912687. Acesso em: 28 ago. 2024.
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      Ryde, N., Gustafsson, B., Edvardsson, B., Meléndez Moreno, J. L., Alves-Brito, A., Asplund, M., et al. (2010). Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra. Astronomy & Astrophysics, 509, A20/1-A20/15. doi:10.1051/0004-6361/200912687
    • NLM

      Ryde N, Gustafsson B, Edvardsson B, Meléndez Moreno JL, Alves-Brito A, Asplund M, Barbuy BLS, Hill V, Käufl HU, Minniti D, Ortolani S, Renzini A, Zoccali M. Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra [Internet]. Astronomy & Astrophysics. 2010 ; 509 A20/1-A20/15.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/200912687
    • Vancouver

      Ryde N, Gustafsson B, Edvardsson B, Meléndez Moreno JL, Alves-Brito A, Asplund M, Barbuy BLS, Hill V, Käufl HU, Minniti D, Ortolani S, Renzini A, Zoccali M. Chemical abundances for 11 bulge stars from high-resolutions, near-IR spectra [Internet]. Astronomy & Astrophysics. 2010 ; 509 A20/1-A20/15.[citado 2024 ago. 28 ] Available from: https://doi.org/10.1051/0004-6361/200912687

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