Filtros : "Ortolani, S" Limpar

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  • 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: 24 abr. 2024.
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      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 abr. 24 ]
    • 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 abr. 24 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: GALÁXIA(VIA LÁCTEA), AGLOMERADOS (GALÁXIA)

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      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. Segue 3: the youngest globular cluster in the outer halo. Monthly Notices of the Royal Astronomical Society, v. 433, p. 1966-1969, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt865. Acesso em: 24 abr. 2024.
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      Ortolani, S., Bica, E., & Barbuy, B. L. S. (2013). Segue 3: the youngest globular cluster in the outer halo. Monthly Notices of the Royal Astronomical Society, 433, 1966-1969. doi:10.1093/mnras/stt865
    • NLM

      Ortolani S, Bica E, Barbuy BLS. Segue 3: the youngest globular cluster in the outer halo [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 433 1966-1969.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stt865
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. Segue 3: the youngest globular cluster in the outer halo [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 433 1966-1969.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1093/mnras/stt865
  • 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: 24 abr. 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 abr. 24 ] 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 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201321943
  • 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: 24 abr. 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 abr. 24 ] 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 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201118138
  • Source: The Astronomical Journal. Unidade: IAG

    Subjects: AGLOMERADOS (GALÁXIA), FOTOMETRIA, GALÁXIA (VIA LÁCTEA)

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      ORTOLANI, S et al. Kronberger 49: a new low-mass globular cluster or an unprecedented bulge window?. The Astronomical Journal, v. 144, p. 147/1-147/11, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-6256/144/5/147. Acesso em: 24 abr. 2024.
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      Ortolani, S., Bonatto, C., Bica, E., Barbuy, B. L. S., & Saito, R. K. (2012). Kronberger 49: a new low-mass globular cluster or an unprecedented bulge window? The Astronomical Journal, 144, 147/1-147/11. doi:10.1088/0004-6256/144/5/147
    • NLM

      Ortolani S, Bonatto C, Bica E, Barbuy BLS, Saito RK. Kronberger 49: a new low-mass globular cluster or an unprecedented bulge window? [Internet]. The Astronomical Journal. 2012 ; 144 147/1-147/11.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1088/0004-6256/144/5/147
    • Vancouver

      Ortolani S, Bonatto C, Bica E, Barbuy BLS, Saito RK. Kronberger 49: a new low-mass globular cluster or an unprecedented bulge window? [Internet]. The Astronomical Journal. 2012 ; 144 147/1-147/11.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1088/0004-6256/144/5/147
  • 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: 24 abr. 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 abr. 24 ] 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 abr. 24 ] 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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      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: 24 abr. 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 abr. 24 ] 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 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/201116548
  • 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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      BARBUY, Beatriz Leonor Silveira et al. Metal-poor globular clusters of the galactic bulge. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 24 abr. 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 abr. 24 ]
    • 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 abr. 24 ]
  • Source: Monthly Notices of The Royal Astronomical Society. Unidade: IAG

    Subjects: ESTRUTURA DA GALÁXIA, GALÁXIA (VIA LÁCTEA)

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      BONATTO, C et al. Open cluster survival within the solar circle: Teutsch 145 and Teutsch 146. Monthly Notices of The Royal Astronomical Society, v. 402, p. 1685-1692, 2010Tradução . . Acesso em: 24 abr. 2024.
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      Bonatto, C., Barbuy, B. L. S., Ortolani, S., & Bica, E. (2010). Open cluster survival within the solar circle: Teutsch 145 and Teutsch 146. Monthly Notices of The Royal Astronomical Society, 402, 1685-1692.
    • NLM

      Bonatto C, Barbuy BLS, Ortolani S, Bica E. Open cluster survival within the solar circle: Teutsch 145 and Teutsch 146. Monthly Notices of The Royal Astronomical Society. 2010 ; 402 1685-1692.[citado 2024 abr. 24 ]
    • Vancouver

      Bonatto C, Barbuy BLS, Ortolani S, Bica E. Open cluster survival within the solar circle: Teutsch 145 and Teutsch 146. Monthly Notices of The Royal Astronomical Society. 2010 ; 402 1685-1692.[citado 2024 abr. 24 ]
  • 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: 24 abr. 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 abr. 24 ] 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 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/200912687
  • Source: Globular clusters: guides to galaxies. Unidade: IAG

    Subjects: AGLOMERADOS (GALÁXIA), GALÁXIA (VIA LÁCTEA)

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      BONATO, C et al. Globular cluster system and Milky Way properties revisited. Globular clusters: guides to galaxies. Tradução . Heidelberg: Springer Berlin, 2009. . . Acesso em: 24 abr. 2024.
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      Bonato, C., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2009). Globular cluster system and Milky Way properties revisited. In Globular clusters: guides to galaxies. Heidelberg: Springer Berlin.
    • NLM

      Bonato C, Barbuy BLS, Bica E, Ortolani S. Globular cluster system and Milky Way properties revisited. In: Globular clusters: guides to galaxies. Heidelberg: Springer Berlin; 2009. [citado 2024 abr. 24 ]
    • Vancouver

      Bonato C, Barbuy BLS, Bica E, Ortolani S. Globular cluster system and Milky Way properties revisited. In: Globular clusters: guides to galaxies. Heidelberg: Springer Berlin; 2009. [citado 2024 abr. 24 ]
  • Source: Globular clusters: guides to galaxies. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), METAIS

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      BARBUY, Beatriz Leonor Silveira et al. Metal-poor globular clusters of the galactic bulge. Globular clusters: guides to galaxies. Tradução . Heidelberg: Springer Berlin, 2009. . . Acesso em: 24 abr. 2024.
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      Barbuy, B. L. S., Zocali, M., Ortolani, S., Momany, Y., Minniti, D., Hill, V., et al. (2009). Metal-poor globular clusters of the galactic bulge. In Globular clusters: guides to galaxies. Heidelberg: Springer Berlin.
    • NLM

      Barbuy BLS, Zocali M, Ortolani S, Momany Y, Minniti D, Hill V, Renzini A, Bica E, Alves-Brito A, Gómez A, Pasquini L, Rich RM. Metal-poor globular clusters of the galactic bulge. In: Globular clusters: guides to galaxies. Heidelberg: Springer Berlin; 2009. [citado 2024 abr. 24 ]
    • Vancouver

      Barbuy BLS, Zocali M, Ortolani S, Momany Y, Minniti D, Hill V, Renzini A, Bica E, Alves-Brito A, Gómez A, Pasquini L, Rich RM. Metal-poor globular clusters of the galactic bulge. In: Globular clusters: guides to galaxies. Heidelberg: Springer Berlin; 2009. [citado 2024 abr. 24 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS, METAIS

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      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: 24 abr. 2024.
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      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 abr. 24 ]
    • 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 abr. 24 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: AGLOMERADOS (GALÁXIA), ASTROFÍSICA ESTELAR

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      BONATTO, C et al. Further proibing the nature of FSR 1767. Monthly Notices of the Royal Astronomical Society, v. 397, n. 2, p. 1032-1040, 2009Tradução . . Acesso em: 24 abr. 2024.
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      Bonatto, C., Barbuy, B. L. S., Bica, E., & Ortolani, S. (2009). Further proibing the nature of FSR 1767. Monthly Notices of the Royal Astronomical Society, 397( 2), 1032-1040.
    • NLM

      Bonatto C, Barbuy BLS, Bica E, Ortolani S. Further proibing the nature of FSR 1767. Monthly Notices of the Royal Astronomical Society. 2009 ; 397( 2): 1032-1040.[citado 2024 abr. 24 ]
    • Vancouver

      Bonatto C, Barbuy BLS, Bica E, Ortolani S. Further proibing the nature of FSR 1767. Monthly Notices of the Royal Astronomical Society. 2009 ; 397( 2): 1032-1040.[citado 2024 abr. 24 ]
  • Source: The Astronomical Journal. Unidade: IAG

    Subjects: AGLOMERADOS (GALÁXIA), ASTROFÍSICA ESTELAR

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      ORTOLANI, S et al. Pfleiderer 2: identification of a new globular cluster in the galaxy. The Astronomical Journal, v. 138, p. 889-894, 2009Tradução . . Acesso em: 24 abr. 2024.
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      Ortolani, S., Barbuy, B. L. S., Bica, E., & Bonatto, C. (2009). Pfleiderer 2: identification of a new globular cluster in the galaxy. The Astronomical Journal, 138, 889-894.
    • NLM

      Ortolani S, Barbuy BLS, Bica E, Bonatto C. Pfleiderer 2: identification of a new globular cluster in the galaxy. The Astronomical Journal. 2009 ; 138 889-894.[citado 2024 abr. 24 ]
    • Vancouver

      Ortolani S, Barbuy BLS, Bica E, Bonatto C. Pfleiderer 2: identification of a new globular cluster in the galaxy. The Astronomical Journal. 2009 ; 138 889-894.[citado 2024 abr. 24 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, GALÁXIA (VIA LÁCTEA)

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      GONZÁLEZ, O. A et al. Li-rich giant branch stars in the Galactic bulge. Astronomy & Astrophysics, v. 508, p. 298-295, 2009Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/200912469. Acesso em: 24 abr. 2024.
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      González, O. A., Zoccali, M., Monaco, L., Hill, V., Cassisi, S., Minniti, D., et al. (2009). Li-rich giant branch stars in the Galactic bulge. Astronomy & Astrophysics, 508, 298-295. doi:10.1051/0004-6361/200912469
    • NLM

      González OA, Zoccali M, Monaco L, Hill V, Cassisi S, Minniti D, Renzini A, Barbuy BLS, Ortolani S, Gomez A. Li-rich giant branch stars in the Galactic bulge [Internet]. Astronomy & Astrophysics. 2009 ; 508 298-295.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/200912469
    • Vancouver

      González OA, Zoccali M, Monaco L, Hill V, Cassisi S, Minniti D, Renzini A, Barbuy BLS, Ortolani S, Gomez A. Li-rich giant branch stars in the Galactic bulge [Internet]. Astronomy & Astrophysics. 2009 ; 508 298-295.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1051/0004-6361/200912469
  • Source: Memorie della Società Astronomica Italiana. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ABUNDÂNCIAS (ASTRONOMIA), GALÁXIAS

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      ZOCCALI, M et al. Chemical abundance in the Galactic bulge. Memorie della Società Astronomica Italiana, v. 79, p. 503-507, 2008Tradução . . Acesso em: 24 abr. 2024.
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      Zoccali, M., Lecureur, A., Hill, V., Barbuy, B. L. S., Renzini, A., Minniti, D., et al. (2008). Chemical abundance in the Galactic bulge. Memorie della Società Astronomica Italiana, 79, 503-507.
    • NLM

      Zoccali M, Lecureur A, Hill V, Barbuy BLS, Renzini A, Minniti D, Gómez A, Ortolani S. Chemical abundance in the Galactic bulge. Memorie della Società Astronomica Italiana. 2008 ; 79 503-507.[citado 2024 abr. 24 ]
    • Vancouver

      Zoccali M, Lecureur A, Hill V, Barbuy BLS, Renzini A, Minniti D, Gómez A, Ortolani S. Chemical abundance in the Galactic bulge. Memorie della Società Astronomica Italiana. 2008 ; 79 503-507.[citado 2024 abr. 24 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: INSTRUMENTAÇÃO (ASTRONOMIA), FOTOMETRIA, POPULAÇÕES ESTELARES, AGLOMERADOS (GALÁXIA)

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      MOMANY, Y et al. Multi-conjugate adaptive optics VLT imaging of the distant old open cluster FSR 1415. Monthly Notices of the Royal Astronomical Society, v. 391, p. 1650-1658, 2008Tradução . . Acesso em: 24 abr. 2024.
    • APA

      Momany, Y., Ortolani, S., Bonatto, C., Bica, E., & Barbuy, B. L. S. (2008). Multi-conjugate adaptive optics VLT imaging of the distant old open cluster FSR 1415. Monthly Notices of the Royal Astronomical Society, 391, 1650-1658.
    • NLM

      Momany Y, Ortolani S, Bonatto C, Bica E, Barbuy BLS. Multi-conjugate adaptive optics VLT imaging of the distant old open cluster FSR 1415. Monthly Notices of the Royal Astronomical Society. 2008 ; 391 1650-1658.[citado 2024 abr. 24 ]
    • Vancouver

      Momany Y, Ortolani S, Bonatto C, Bica E, Barbuy BLS. Multi-conjugate adaptive optics VLT imaging of the distant old open cluster FSR 1415. Monthly Notices of the Royal Astronomical Society. 2008 ; 391 1650-1658.[citado 2024 abr. 24 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: AGLOMERADOS DE GALÁXIAS

    Acesso à fonteDOIHow to cite
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    • ABNT

      ORTOLANI, S e BICA, E e BARBUY, Beatriz Leonor Silveira. The old metal-poor open cluster ESO 92-SC05: accreted from a dwarf galaxy?. Monthly Notices of the Royal Astronomical Society, v. 388, p. 723-728, 2008Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2008.13427.x. Acesso em: 24 abr. 2024.
    • APA

      Ortolani, S., Bica, E., & Barbuy, B. L. S. (2008). The old metal-poor open cluster ESO 92-SC05: accreted from a dwarf galaxy? Monthly Notices of the Royal Astronomical Society, 388, 723-728. doi:10.1111/j.1365-2966.2008.13427.x
    • NLM

      Ortolani S, Bica E, Barbuy BLS. The old metal-poor open cluster ESO 92-SC05: accreted from a dwarf galaxy? [Internet]. Monthly Notices of the Royal Astronomical Society. 2008 ; 388 723-728.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1111/j.1365-2966.2008.13427.x
    • Vancouver

      Ortolani S, Bica E, Barbuy BLS. The old metal-poor open cluster ESO 92-SC05: accreted from a dwarf galaxy? [Internet]. Monthly Notices of the Royal Astronomical Society. 2008 ; 388 723-728.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1111/j.1365-2966.2008.13427.x
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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

      ZOCCALI, M et al. The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics, v. 486, p. 177-189, 2008Tradução . . Acesso em: 24 abr. 2024.
    • APA

      Zoccali, M., Hill, V., Lecureur, A., Barbuy, B. L. S., Renzini, A., Minniti, D., et al. (2008). The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics, 486, 177-189.
    • NLM

      Zoccali M, Hill V, Lecureur A, Barbuy BLS, Renzini A, Minniti D, Gómez A, Ortolani S. The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics. 2008 ; 486 177-189.[citado 2024 abr. 24 ]
    • Vancouver

      Zoccali M, Hill V, Lecureur A, Barbuy BLS, Renzini A, Minniti D, Gómez A, Ortolani S. The metal content of bulge field stars from FLAMES-GIRAFFE spectra: I. Stellar parameters and iron abundances. Astronomy & Astrophysics. 2008 ; 486 177-189.[citado 2024 abr. 24 ]

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