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  • 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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201833953
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, NUVENS DE MAGALHÃES

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    • ABNT

      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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, CENTRO GALÁCTICO

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, v. 591, p. A53/1-A53/14, 2016Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201628106. Acesso em: 10 jun. 2024.
    • APA

      Barbuy, B. L. S., Cantelli, E., Vemado, A., Ernandes, H., Ortoloni, S., Saviane, I., et al. (2016). High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1. Astronomy & Astrophysics, 591, A53/1-A53/14. doi:10.1051/0004-6361/201628106
    • NLM

      Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201628106
    • Vancouver

      Barbuy BLS, Cantelli E, Vemado A, Ernandes H, Ortoloni S, Saviane I, Bica E, Minniti D, Dias B, Momany Y, Hill V, Zoccali M, Siqueira Mello C. High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP1 [Internet]. Astronomy & Astrophysics. 2016 ;591 A53/1-A53/14.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201628106
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS, NUVENS DE MAGALHÃES

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    • ABNT

      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: 10 jun. 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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201527558
  • 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 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: 10 jun. 2024.
    • APA

      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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201424311
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), GALÁXIAS

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    • ABNT

      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: 10 jun. 2024.
    • APA

      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 jun. 10 ] 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 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361/201321943
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS, METAIS

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. VLT - Flames analysis of 8 giants in the bulge metal-poor globular cluster NGC 6522: oldest cluster in the Galaxy ?. Astronomy & Astrophysics, v. 507, p. 405-415, 2009Tradução . . Acesso em: 10 jun. 2024.
    • APA

      Barbuy, B. L. S., Zoccali, M., Ortolani, S., Hill, V., Minniti, D., Bica, E., et al. (2009). VLT - Flames analysis of 8 giants in the bulge metal-poor globular cluster NGC 6522: oldest cluster in the Galaxy ? Astronomy & Astrophysics, 507, 405-415.
    • NLM

      Barbuy BLS, Zoccali M, Ortolani S, Hill V, Minniti D, Bica E, Renzini A, Gómez A. VLT - Flames analysis of 8 giants in the bulge metal-poor globular cluster NGC 6522: oldest cluster in the Galaxy ? Astronomy & Astrophysics. 2009 ; 507 405-415.[citado 2024 jun. 10 ]
    • Vancouver

      Barbuy BLS, Zoccali M, Ortolani S, Hill V, Minniti D, Bica E, Renzini A, Gómez A. VLT - Flames analysis of 8 giants in the bulge metal-poor globular cluster NGC 6522: oldest cluster in the Galaxy ? Astronomy & Astrophysics. 2009 ; 507 405-415.[citado 2024 jun. 10 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics, v. 449, p. 349-358, 2006Tradução . . Acesso em: 10 jun. 2024.
    • APA

      Barbuy, B. L. S., Zoccali, M., Ortolani, S., Momany, Y., Minniti, D., Hill, V., et al. (2006). VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics, 449, 349-358.
    • NLM

      Barbuy BLS, Zoccali M, Ortolani S, Momany Y, Minniti D, Hill V, Renzini A, Rich RM, Bica E, Pasquini L, Yadav KS. VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics. 2006 ; 449 349-358.[citado 2024 jun. 10 ]
    • Vancouver

      Barbuy BLS, Zoccali M, Ortolani S, Momany Y, Minniti D, Hill V, Renzini A, Rich RM, Bica E, Pasquini L, Yadav KS. VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1: analysis of two giants in HP-1. Astronomy and Astrophysics. 2006 ; 449 349-358.[citado 2024 jun. 10 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ASTRONOMIA

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    • ABNT

      BONATTO, C et al. Detection of Ks-excess stars in the 14 Myr open cluster NGC 4755. Astronomy and Astrophysics, v. 453, p. 121-132, 2006Tradução . . Acesso em: 10 jun. 2024.
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      Bonatto, C., Bica, E., Ortolani, S., & Barbuy, B. L. S. (2006). Detection of Ks-excess stars in the 14 Myr open cluster NGC 4755. Astronomy and Astrophysics, 453, 121-132.
    • NLM

      Bonatto C, Bica E, Ortolani S, Barbuy BLS. Detection of Ks-excess stars in the 14 Myr open cluster NGC 4755. Astronomy and Astrophysics. 2006 ; 453 121-132.[citado 2024 jun. 10 ]
    • Vancouver

      Bonatto C, Bica E, Ortolani S, Barbuy BLS. Detection of Ks-excess stars in the 14 Myr open cluster NGC 4755. Astronomy and Astrophysics. 2006 ; 453 121-132.[citado 2024 jun. 10 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: GALÁXIAS

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    • ABNT

      BICA, E et al. Globular cluster system and Milky Way properties revisited. Astronomy and Astrophysics, v. 450, p. 105-115, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20054351. Acesso em: 10 jun. 2024.
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      Bica, E., Bonatto, C., Barbuy, B. L. S., & Ortolani, S. (2006). Globular cluster system and Milky Way properties revisited. Astronomy and Astrophysics, 450, 105-115. doi:10.1051/0004-6361:20054351
    • NLM

      Bica E, Bonatto C, Barbuy BLS, Ortolani S. Globular cluster system and Milky Way properties revisited [Internet]. Astronomy and Astrophysics. 2006 ; 450 105-115.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20054351
    • Vancouver

      Bica E, Bonatto C, Barbuy BLS, Ortolani S. Globular cluster system and Milky Way properties revisited [Internet]. Astronomy and Astrophysics. 2006 ; 450 105-115.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20054351
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. SOAR BVI photometry of the metal-poor bulge globular cluster NGC 6642. Astronomy and Astrophysics, v. 449, p. 1019-1024, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20054073. Acesso em: 10 jun. 2024.
    • APA

      Barbuy, B. L. S., Bica, E., Ortolani, S., & Bonatto, C. (2006). SOAR BVI photometry of the metal-poor bulge globular cluster NGC 6642. Astronomy and Astrophysics, 449, 1019-1024. doi:10.1051/0004-6361:20054073
    • NLM

      Barbuy BLS, Bica E, Ortolani S, Bonatto C. SOAR BVI photometry of the metal-poor bulge globular cluster NGC 6642 [Internet]. Astronomy and Astrophysics. 2006 ; 449 1019-1024.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20054073
    • Vancouver

      Barbuy BLS, Bica E, Ortolani S, Bonatto C. SOAR BVI photometry of the metal-poor bulge globular cluster NGC 6642 [Internet]. Astronomy and Astrophysics. 2006 ; 449 1019-1024.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20054073
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, GALÁXIAS

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      BRITO, A. Alves et al. VLT-UVES abundance analysis of four giants in NGC 6553. Astronomy and Astrophysics, v. 460, p. 269-276, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065488. Acesso em: 10 jun. 2024.
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      Brito, A. A., Barbuy, B. L. S., Zoccali, M., Minniti, D., Ortolani, S., Hill, V., et al. (2006). VLT-UVES abundance analysis of four giants in NGC 6553. Astronomy and Astrophysics, 460, 269-276. doi:10.1051/0004-6361:20065488
    • NLM

      Brito AA, Barbuy BLS, Zoccali M, Minniti D, Ortolani S, Hill V, Renzini A, Pasquini L, Bica E, Rich RM, Meléndez J, Momany Y. VLT-UVES abundance analysis of four giants in NGC 6553 [Internet]. Astronomy and Astrophysics. 2006 ; 460 269-276.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20065488
    • Vancouver

      Brito AA, Barbuy BLS, Zoccali M, Minniti D, Ortolani S, Hill V, Renzini A, Pasquini L, Bica E, Rich RM, Meléndez J, Momany Y. VLT-UVES abundance analysis of four giants in NGC 6553 [Internet]. Astronomy and Astrophysics. 2006 ; 460 269-276.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20065488
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ABUNDÂNCIA ESTELAR

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      ALVES-BRITO, Alan et al. VLT-UVES analysis of 5 giants in 47 Tucanae. Astronomy and Astrophysics, v. 435, p. 657-667, 2005Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20041634. Acesso em: 10 jun. 2024.
    • APA

      Alves-Brito, A., Barbuy, B. L. S., Ortolani, S., Momany, Y., Hill, V., Zoccali, M., et al. (2005). VLT-UVES analysis of 5 giants in 47 Tucanae. Astronomy and Astrophysics, 435, 657-667. doi:10.1051/0004-6361:20041634
    • NLM

      Alves-Brito A, Barbuy BLS, Ortolani S, Momany Y, Hill V, Zoccali M, Renzini A, Minniti D, Pasquini L, Bica E, Rich RM. VLT-UVES analysis of 5 giants in 47 Tucanae [Internet]. Astronomy and Astrophysics. 2005 ; 435 657-667.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041634
    • Vancouver

      Alves-Brito A, Barbuy BLS, Ortolani S, Momany Y, Hill V, Zoccali M, Renzini A, Minniti D, Pasquini L, Bica E, Rich RM. VLT-UVES analysis of 5 giants in 47 Tucanae [Internet]. Astronomy and Astrophysics. 2005 ; 435 657-667.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041634
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ASTROFÍSICA ESTELAR

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      ORTOLANI, S et al. The old openclusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34). Astronomy and Astrophysics, v. 429, p. 607-612, 2005Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20041458. Acesso em: 10 jun. 2024.
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      Ortolani, S., Bica, E., Barbuy, B. L. S., & Zoccali, M. (2005). The old openclusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34). Astronomy and Astrophysics, 429, 607-612. doi:10.1051/0004-6361:20041458
    • NLM

      Ortolani S, Bica E, Barbuy BLS, Zoccali M. The old openclusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34) [Internet]. Astronomy and Astrophysics. 2005 ; 429 607-612.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041458
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS, Zoccali M. The old openclusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34) [Internet]. Astronomy and Astrophysics. 2005 ; 429 607-612.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041458
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: GALÁXIAS

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      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. Colour-Magnitude analysis of five old open clusters. Astronomy and Astrophysics, p. V. 437 531-536, 2005Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20042326. Acesso em: 10 jun. 2024.
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      Ortolani, S., Bica, E., & Barbuy, B. L. S. (2005). Colour-Magnitude analysis of five old open clusters. Astronomy and Astrophysics, V. 437 531-536. doi:10.1051/0004-6361:20042326
    • NLM

      Ortolani S, Bica E, Barbuy BLS. Colour-Magnitude analysis of five old open clusters [Internet]. Astronomy and Astrophysics. 2005 ;V. 437 531-536.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20042326
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. Colour-Magnitude analysis of five old open clusters [Internet]. Astronomy and Astrophysics. 2005 ;V. 437 531-536.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20042326
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ASTROFÍSICA ESTELAR

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      ORTOLANI, Sérgio et al. The old open clusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34). Astronomy and Astrophysics, v. 429, p. 607-612, 2004Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20041458. Acesso em: 10 jun. 2024.
    • APA

      Ortolani, S., Bica, E., Barbuy, B. L. S., & Zoccali, M. (2004). The old open clusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34). Astronomy and Astrophysics, 429, 607-612. doi:10.1051/0004-6361:20041458
    • NLM

      Ortolani S, Bica E, Barbuy BLS, Zoccali M. The old open clusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34) [Internet]. Astronomy and Astrophysics. 2004 ; 429 607-612.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041458
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS, Zoccali M. The old open clusters Berkeley 36, Berkeley 73 and Biurakan 13 (Berkeley 34) [Internet]. Astronomy and Astrophysics. 2004 ; 429 607-612.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041458
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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      ZOCCALI, M et al. The metal content of the bulge globular cluster NGC 6528. Astronomy and Astrophysics, v. 423, p. 507-516, 2004Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20041014. Acesso em: 10 jun. 2024.
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      Zoccali, M., Barbuy, B. L. S., Hill, S., Ortoloni, S., Renzini, A., Bica, E., et al. (2004). The metal content of the bulge globular cluster NGC 6528. Astronomy and Astrophysics, 423, 507-516. doi:10.1051/0004-6361:20041014
    • NLM

      Zoccali M, Barbuy BLS, Hill S, Ortoloni S, Renzini A, Bica E, Momany Y, Pasquini L, Minniti D, Rich RM. The metal content of the bulge globular cluster NGC 6528 [Internet]. Astronomy and Astrophysics. 2004 ; 423 507-516.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041014
    • Vancouver

      Zoccali M, Barbuy BLS, Hill S, Ortoloni S, Renzini A, Bica E, Momany Y, Pasquini L, Minniti D, Rich RM. The metal content of the bulge globular cluster NGC 6528 [Internet]. Astronomy and Astrophysics. 2004 ; 423 507-516.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20041014
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: GALÁXIAS

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      DUTRA, C.M et al. On the calibration of the COBE/IRAS dust emission reddening maps. Astronomy and Astrophysics, v. 408, p. 287-295, 2003Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20030980. Acesso em: 10 jun. 2024.
    • APA

      Dutra, C. M., Ahumada, V., Clariá, J. J., Bica, E., & Barbuy, B. L. S. (2003). On the calibration of the COBE/IRAS dust emission reddening maps. Astronomy and Astrophysics, 408, 287-295. doi:10.1051/0004-6361:20030980
    • NLM

      Dutra CM, Ahumada V, Clariá JJ, Bica E, Barbuy BLS. On the calibration of the COBE/IRAS dust emission reddening maps [Internet]. Astronomy and Astrophysics. 2003 ;408 287-295.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20030980
    • Vancouver

      Dutra CM, Ahumada V, Clariá JJ, Bica E, Barbuy BLS. On the calibration of the COBE/IRAS dust emission reddening maps [Internet]. Astronomy and Astrophysics. 2003 ;408 287-295.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20030980
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: GALÁXIAS

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      DUTRA, C.M et al. NTT infrared imaging of star cluster candidates towards the central parts of the galaxy. Astronomy and Astrophysics, v. 408, p. 127-134, 2003Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20030944. Acesso em: 10 jun. 2024.
    • APA

      Dutra, C. M., Ortolani, S., Bica, E., Barbuy, B. L. S., Zoccali, M., & Momany, Y. (2003). NTT infrared imaging of star cluster candidates towards the central parts of the galaxy. Astronomy and Astrophysics, 408, 127-134. doi:10.1051/0004-6361:20030944
    • NLM

      Dutra CM, Ortolani S, Bica E, Barbuy BLS, Zoccali M, Momany Y. NTT infrared imaging of star cluster candidates towards the central parts of the galaxy [Internet]. Astronomy and Astrophysics. 2003 ;408 127-134.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20030944
    • Vancouver

      Dutra CM, Ortolani S, Bica E, Barbuy BLS, Zoccali M, Momany Y. NTT infrared imaging of star cluster candidates towards the central parts of the galaxy [Internet]. Astronomy and Astrophysics. 2003 ;408 127-134.[citado 2024 jun. 10 ] Available from: https://doi.org/10.1051/0004-6361:20030944
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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      MELÉNDEZ, J et al. Gemini-phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553*. Astronomy and Astrophysics, v. 411, p. 417-426, 2003Tradução . . Acesso em: 10 jun. 2024.
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      Meléndez, J., Barbuy, B. L. S., Bica, E., Zoccali, M., Ortolani, S., Renzini, A., & Hill, V. (2003). Gemini-phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553*. Astronomy and Astrophysics, 411, 417-426.
    • NLM

      Meléndez J, Barbuy BLS, Bica E, Zoccali M, Ortolani S, Renzini A, Hill V. Gemini-phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553*. Astronomy and Astrophysics. 2003 ;411 417-426.[citado 2024 jun. 10 ]
    • Vancouver

      Meléndez J, Barbuy BLS, Bica E, Zoccali M, Ortolani S, Renzini A, Hill V. Gemini-phoenix infrared high-resolution abundance analysis of five giants in the bulge globular cluster NGC 6553*. Astronomy and Astrophysics. 2003 ;411 417-426.[citado 2024 jun. 10 ]

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