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  • 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: 11 out. 2024.
    • APA

      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 out. 11 ] 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 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201833525
  • 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: 11 out. 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 out. 11 ] 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 out. 11 ] 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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    • ABNT

      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: 11 out. 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 out. 11 ] 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 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/201423996
  • 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: 11 out. 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 out. 11 ] 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 out. 11 ] 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: 11 out. 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 out. 11 ] 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 out. 11 ] 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: NUVENS DE MAGALHÃES, ESTRELAS

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    • ABNT

      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: 11 out. 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 out. 11 ]
    • 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 out. 11 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      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: 11 out. 2024.
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      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 out. 11 ] 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 out. 11 ] 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: 11 out. 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 out. 11 ] 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 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/200913757
  • Source: Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, AGLOMERADOS (GALÁXIA), ABUNDÂNCIAS (ASTRONOMIA)

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. Metal-poor globular clusters of the galactic bulge. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 11 out. 2024.
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      Barbuy, B. L. S., Ortolani, S., Zoccali, M., Hill, V., Minniti, D., Bica, E., et al. (2010). Metal-poor globular clusters of the galactic bulge. In Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Cambridge: Cambridge University Press.
    • NLM

      Barbuy BLS, Ortolani S, Zoccali M, Hill V, Minniti D, Bica E, Renzini A, Gómez A. Metal-poor globular clusters of the galactic bulge. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 out. 11 ]
    • Vancouver

      Barbuy BLS, Ortolani S, Zoccali M, Hill V, Minniti D, Bica E, Renzini A, Gómez A. Metal-poor globular clusters of the galactic bulge. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 out. 11 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

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

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      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: 11 out. 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 out. 11 ] 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 out. 11 ] Available from: https://doi.org/10.1051/0004-6361/200912687
  • Source: Memorie della Società Astronomica Italiana. Unidade: IAG

    Subjects: ESTRELAS, FOTOMETRIA, POPULAÇÕES ESTELARES, AGLOMERADOS (GALÁXIA)

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      ORTOLANI, S et al. New low latitude globular clusters. Memorie della Società Astronomica Italiana, v. 79, p. 352-354, 2008Tradução . . Acesso em: 11 out. 2024.
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      Ortolani, S., Bica, E., Barbuy, B. L. S., & Bonatto, C. (2008). New low latitude globular clusters. Memorie della Società Astronomica Italiana, 79, 352-354.
    • NLM

      Ortolani S, Bica E, Barbuy BLS, Bonatto C. New low latitude globular clusters. Memorie della Società Astronomica Italiana. 2008 ; 79 352-354.[citado 2024 out. 11 ]
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS, Bonatto C. New low latitude globular clusters. Memorie della Società Astronomica Italiana. 2008 ; 79 352-354.[citado 2024 out. 11 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS

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      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: 11 out. 2024.
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      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 out. 11 ]
    • 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 out. 11 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS

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      ZOCCALI, M et al. Oxygen abundances in the galactic bulge: evidence for fast chemical enrichment. Astronomy and Astrophysics, v. 457, p. L1-L4, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065659. Acesso em: 11 out. 2024.
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      Zoccali, M., Lecureur, A., Barbuy, B. L. S., Hill, V., Renzini, A., Minniti, D., et al. (2006). Oxygen abundances in the galactic bulge: evidence for fast chemical enrichment. Astronomy and Astrophysics, 457, L1-L4. doi:10.1051/0004-6361:20065659
    • NLM

      Zoccali M, Lecureur A, Barbuy BLS, Hill V, Renzini A, Minniti D, Momany Y, Gómez A, Ortolani S. Oxygen abundances in the galactic bulge: evidence for fast chemical enrichment [Internet]. Astronomy and Astrophysics. 2006 ; 457 L1-L4.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361:20065659
    • Vancouver

      Zoccali M, Lecureur A, Barbuy BLS, Hill V, Renzini A, Minniti D, Momany Y, Gómez A, Ortolani S. Oxygen abundances in the galactic bulge: evidence for fast chemical enrichment [Internet]. Astronomy and Astrophysics. 2006 ; 457 L1-L4.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/0004-6361:20065659
  • Source: Astronomy and Astrophysics Supplement Series. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS

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      BICA, E e ORTOLANI, S e BARBUY, Beatriz Leonor Silveira. The nature of the star clusters ESO 93-SC08 and ESO 452-SC11*. Astronomy and Astrophysics Supplement Series, v. 136, n. 2, p. 363-372, 1999Tradução . . Acesso em: 11 out. 2024.
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      Bica, E., Ortolani, S., & Barbuy, B. L. S. (1999). The nature of the star clusters ESO 93-SC08 and ESO 452-SC11*. Astronomy and Astrophysics Supplement Series, 136( 2), 363-372.
    • NLM

      Bica E, Ortolani S, Barbuy BLS. The nature of the star clusters ESO 93-SC08 and ESO 452-SC11*. Astronomy and Astrophysics Supplement Series. 1999 ;136( 2): 363-372.[citado 2024 out. 11 ]
    • Vancouver

      Bica E, Ortolani S, Barbuy BLS. The nature of the star clusters ESO 93-SC08 and ESO 452-SC11*. Astronomy and Astrophysics Supplement Series. 1999 ;136( 2): 363-372.[citado 2024 out. 11 ]
  • Source: Astronomy and Astrophysics Supplement Series. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS

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      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. V, I and Gunn z photometry of faint bulge globular clusters: Terzan 10, ESO 456-SC38 and UKS 1. Astronomy and Astrophysics Supplement Series, v. 126, n. 2, p. 319-324, 1997Tradução . . Acesso em: 11 out. 2024.
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      Ortolani, S., Bica, E., & Barbuy, B. L. S. (1997). V, I and Gunn z photometry of faint bulge globular clusters: Terzan 10, ESO 456-SC38 and UKS 1. Astronomy and Astrophysics Supplement Series, 126( 2), 319-324.
    • NLM

      Ortolani S, Bica E, Barbuy BLS. V, I and Gunn z photometry of faint bulge globular clusters: Terzan 10, ESO 456-SC38 and UKS 1. Astronomy and Astrophysics Supplement Series. 1997 ; 126( 2): 319-324.[citado 2024 out. 11 ]
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. V, I and Gunn z photometry of faint bulge globular clusters: Terzan 10, ESO 456-SC38 and UKS 1. Astronomy and Astrophysics Supplement Series. 1997 ; 126( 2): 319-324.[citado 2024 out. 11 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS

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      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics, v. 326, n. 2, p. 614-619, 1997Tradução . . Acesso em: 11 out. 2024.
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      Ortolani, S., Bica, E., & Barbuy, B. L. S. (1997). V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics, 326( 2), 614-619.
    • NLM

      Ortolani S, Bica E, Barbuy BLS. V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics. 1997 ; 326( 2): 614-619.[citado 2024 out. 11 ]
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. V, I photometry of the metal-rich bulge globular cluster Terzan 2. Astronomy and Astrophysics. 1997 ; 326( 2): 614-619.[citado 2024 out. 11 ]
  • Source: Astronomy and Astrophysics Supplement Series. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS

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      BARBUY, Beatriz Leonor Silveira e ORTOLANI, S e BICA, E. NTT V, I, z photometry of the metal-rich bulge globular cluster Terzan 6. Astronomy and Astrophysics Supplement Series, v. 122, n. 3, p. 483-488, 1997Tradução . . Disponível em: https://doi.org/10.1051/aas:1997148. Acesso em: 11 out. 2024.
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      Barbuy, B. L. S., Ortolani, S., & Bica, E. (1997). NTT V, I, z photometry of the metal-rich bulge globular cluster Terzan 6. Astronomy and Astrophysics Supplement Series, 122( 3), 483-488. doi:10.1051/aas:1997148
    • NLM

      Barbuy BLS, Ortolani S, Bica E. NTT V, I, z photometry of the metal-rich bulge globular cluster Terzan 6 [Internet]. Astronomy and Astrophysics Supplement Series. 1997 ; 122( 3): 483-488.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/aas:1997148
    • Vancouver

      Barbuy BLS, Ortolani S, Bica E. NTT V, I, z photometry of the metal-rich bulge globular cluster Terzan 6 [Internet]. Astronomy and Astrophysics Supplement Series. 1997 ; 122( 3): 483-488.[citado 2024 out. 11 ] Available from: https://doi.org/10.1051/aas:1997148
  • Source: Astronomy and Astrophysics Supplement Series. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS, ASTROFÍSICA ESTELAR

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    • ABNT

      BICA, E e ORTOLANI, S e BARBUY, Beatriz Leonor Silveira. Ntt v, i colour-magnitude diagrams of the bulge globular cluster tonantzintla 2. Astronomy and Astrophysics Supplement Series, v. no 1996, n. 1, p. 153-156, 1996Tradução . . Acesso em: 11 out. 2024.
    • APA

      Bica, E., Ortolani, S., & Barbuy, B. L. S. (1996). Ntt v, i colour-magnitude diagrams of the bulge globular cluster tonantzintla 2. Astronomy and Astrophysics Supplement Series, no 1996( 1), 153-156.
    • NLM

      Bica E, Ortolani S, Barbuy BLS. Ntt v, i colour-magnitude diagrams of the bulge globular cluster tonantzintla 2. Astronomy and Astrophysics Supplement Series. 1996 ; no 1996( 1): 153-156.[citado 2024 out. 11 ]
    • Vancouver

      Bica E, Ortolani S, Barbuy BLS. Ntt v, i colour-magnitude diagrams of the bulge globular cluster tonantzintla 2. Astronomy and Astrophysics Supplement Series. 1996 ; no 1996( 1): 153-156.[citado 2024 out. 11 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS, GALÁXIAS

    How to cite
    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. Ntt v, i; and gunn z colour-magnitude diagrams of liller 1: a globular cluster as metal-rich as the inner bulge stellar population ?. Astronomy and Astrophysics, v. 306, n. 1, p. 134-140, 1996Tradução . . Acesso em: 11 out. 2024.
    • APA

      Ortolani, S., Bica, E., & Barbuy, B. L. S. (1996). Ntt v, i; and gunn z colour-magnitude diagrams of liller 1: a globular cluster as metal-rich as the inner bulge stellar population ? Astronomy and Astrophysics, 306( 1), 134-140.
    • NLM

      Ortolani S, Bica E, Barbuy BLS. Ntt v, i; and gunn z colour-magnitude diagrams of liller 1: a globular cluster as metal-rich as the inner bulge stellar population ? Astronomy and Astrophysics. 1996 ; 306( 1): 134-140.[citado 2024 out. 11 ]
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. Ntt v, i; and gunn z colour-magnitude diagrams of liller 1: a globular cluster as metal-rich as the inner bulge stellar population ? Astronomy and Astrophysics. 1996 ; 306( 1): 134-140.[citado 2024 out. 11 ]
  • Source: Stellar Populations: Proceedings. Conference titles: International Astronomical Union Symposium. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS, ASTROFÍSICA ESTELAR

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    A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. 'ALFA'-elements in bulge stars: arp 1145, terzan 1-2. 1995, Anais.. Dordrecht: Kluwer, 1995. . Acesso em: 11 out. 2024.
    • APA

      Barbuy, B. L. S., Ortolani, S., Renzini, A., Bica, E., & Castro, S. M. (1995). 'ALFA'-elements in bulge stars: arp 1145, terzan 1-2. In Stellar Populations: Proceedings. Dordrecht: Kluwer.
    • NLM

      Barbuy BLS, Ortolani S, Renzini A, Bica E, Castro SM. 'ALFA'-elements in bulge stars: arp 1145, terzan 1-2. Stellar Populations: Proceedings. 1995 ;[citado 2024 out. 11 ]
    • Vancouver

      Barbuy BLS, Ortolani S, Renzini A, Bica E, Castro SM. 'ALFA'-elements in bulge stars: arp 1145, terzan 1-2. Stellar Populations: Proceedings. 1995 ;[citado 2024 out. 11 ]

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