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  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Subjects: MATÉRIA ESCURA, COSMOLOGIA, ESTRUTURA DO UNIVERSO

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      ABRIL, Javier et al. Disentangling cataclysmic variables in Gaia's HR diagram. Monthly Notices of the Royal Astronomical Society, v. 492, n. 1, p. L78–88, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnrasl/slz181. Acesso em: 24 ago. 2024.
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      abril, J., Schmidtobreick, L., Ederoclite, A., & López-Sanjuan, C. (2020). Disentangling cataclysmic variables in Gaia's HR diagram. Monthly Notices of the Royal Astronomical Society, 492( 1), L78–88. doi:10.1093/mnrasl/slz181
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      abril J, Schmidtobreick L, Ederoclite A, López-Sanjuan C. Disentangling cataclysmic variables in Gaia's HR diagram [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 1): L78–88.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1093/mnrasl/slz181
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      abril J, Schmidtobreick L, Ederoclite A, López-Sanjuan C. Disentangling cataclysmic variables in Gaia's HR diagram [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 1): L78–88.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1093/mnrasl/slz181
  • 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: 24 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
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      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. 24 ] Available from: https://doi.org/10.1051/0004-6361/201423996
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      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. 24 ] Available from: https://doi.org/10.1051/0004-6361/201423996
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, GALÁXIAS (INTERAÇÃO), GALÁXIAS ESPIRAIS, FORMAÇÃO DE ESTRELAS

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      EUFRASIO, Rafael T et al. Star formation histories across the interacting galaxy NGC 6872, the largest-known spiral. The Astrophysical Journal, v. 795, p. 89/1-89/14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/795/1/89. Acesso em: 24 ago. 2024.
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      Eufrasio, R. T., Dwek, E., Arendt, R. G., Gadotti, D. A., Urrutia-Viscarra, F., Oliveira, C. L. M. de, & Benford, D. J. (2014). Star formation histories across the interacting galaxy NGC 6872, the largest-known spiral. The Astrophysical Journal, 795, 89/1-89/14. doi:10.1088/0004-637X/795/1/89
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      Eufrasio RT, Dwek E, Arendt RG, Gadotti DA, Urrutia-Viscarra F, Oliveira CLM de, Benford DJ. Star formation histories across the interacting galaxy NGC 6872, the largest-known spiral [Internet]. The Astrophysical Journal. 2014 ; 795 89/1-89/14.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1088/0004-637X/795/1/89
    • Vancouver

      Eufrasio RT, Dwek E, Arendt RG, Gadotti DA, Urrutia-Viscarra F, Oliveira CLM de, Benford DJ. Star formation histories across the interacting galaxy NGC 6872, the largest-known spiral [Internet]. The Astrophysical Journal. 2014 ; 795 89/1-89/14.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1088/0004-637X/795/1/89
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, MÉTODOS NUMÉRICOS, INTERFEROMETRIA

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      DOMICIANO DE SOUZA, A et al. The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI. Astronomy & Astrophysics, v. 569, p. A10/1-A10/15, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201424144. Acesso em: 24 ago. 2024.
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      Domiciano de Souza, A., Kervella, P., Moser Faes, D., Dalla Vedova, G., Mérand, A., Le Bouquin J.-B,, et al. (2014). The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI. Astronomy & Astrophysics, 569, A10/1-A10/15. doi:10.1051/0004-6361/201424144
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      Domiciano de Souza A, Kervella P, Moser Faes D, Dalla Vedova G, Mérand A, Le Bouquin J.-B, Espinosa Lara F, Rieutord M, Bendjoya P, Carciofi AC, Hadjara M, Millour F, Vakili F. The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI [Internet]. Astronomy & Astrophysics. 2014 ; 569 A10/1-A10/15.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201424144
    • Vancouver

      Domiciano de Souza A, Kervella P, Moser Faes D, Dalla Vedova G, Mérand A, Le Bouquin J.-B, Espinosa Lara F, Rieutord M, Bendjoya P, Carciofi AC, Hadjara M, Millour F, Vakili F. The environment of the fast rotating star Achernar: III. Photospheric parameters revealed by the VLTI [Internet]. Astronomy & Astrophysics. 2014 ; 569 A10/1-A10/15.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201424144
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ESTRELAS, PLANETAS, INFRAVERMELHO, INSTRUMENTAÇÃO (ASTRONOMIA), ESTATÍSTICA

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      WAHHAJ, Zahed et al. The Gemini planet-finding campaign: the frequency of giant planets around debris disk stars. The Astrophysical Journal, v. 773, n. 2, p. 179/1-179/30, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/773/2/179. Acesso em: 24 ago. 2024.
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      Wahhaj, Z., Liu, M. C., Nielsen, E. L., Dal Pino, E. M. de G., & Gregorio-Hetem, J. (2013). The Gemini planet-finding campaign: the frequency of giant planets around debris disk stars. The Astrophysical Journal, 773( 2), 179/1-179/30. doi:10.1088/0004-637X/773/2/179
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      Wahhaj Z, Liu MC, Nielsen EL, Dal Pino EM de G, Gregorio-Hetem J. The Gemini planet-finding campaign: the frequency of giant planets around debris disk stars [Internet]. The Astrophysical Journal. 2013 ; 773( 2): 179/1-179/30.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1088/0004-637X/773/2/179
    • Vancouver

      Wahhaj Z, Liu MC, Nielsen EL, Dal Pino EM de G, Gregorio-Hetem J. The Gemini planet-finding campaign: the frequency of giant planets around debris disk stars [Internet]. The Astrophysical Journal. 2013 ; 773( 2): 179/1-179/30.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1088/0004-637X/773/2/179
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS VARIÁVEIS, ESTRELAS, FOTOMETRIA

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      DE MEDEIROS, J. R et al. Overview of semi-sinusoidal stellar veriability with the CoRoT satellite. Astronomy & Astrophysics, v. 555, p. A63/1-A63/12, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201219415. Acesso em: 24 ago. 2024.
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      De Medeiros, J. R., Ferreira Lopes, C. E., Leão, I. C., Martins, B. L. C., Catelan, M., Baglin, A., et al. (2013). Overview of semi-sinusoidal stellar veriability with the CoRoT satellite. Astronomy & Astrophysics, 555, A63/1-A63/12. doi:10.1051/0004-6361/201219415
    • NLM

      De Medeiros JR, Ferreira Lopes CE, Leão IC, Martins BLC, Catelan M, Baglin A, Vieira S, Bravo JP, Cortés C, Freitas DB de, Janot-Pacheco E, Maciel SC, Melo CHF, Osorio Y, Porto de Mello GF, Valio A. Overview of semi-sinusoidal stellar veriability with the CoRoT satellite [Internet]. Astronomy & Astrophysics. 2013 ; 555 A63/1-A63/12.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201219415
    • Vancouver

      De Medeiros JR, Ferreira Lopes CE, Leão IC, Martins BLC, Catelan M, Baglin A, Vieira S, Bravo JP, Cortés C, Freitas DB de, Janot-Pacheco E, Maciel SC, Melo CHF, Osorio Y, Porto de Mello GF, Valio A. Overview of semi-sinusoidal stellar veriability with the CoRoT satellite [Internet]. Astronomy & Astrophysics. 2013 ; 555 A63/1-A63/12.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201219415
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ESTRELAS, ASTROFÍSICA ESTELAR

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      RIVINIUS, Th et al. Variable rotational line broadening in the Be star Achernar. Astronomy & Astrophysics, v. 559, 2013Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201322515. Acesso em: 24 ago. 2024.
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      Rivinius, T., Baade, D., Townsend, R. H. D., Carciofi, A. C., & Stefl, S. (2013). Variable rotational line broadening in the Be star Achernar. Astronomy & Astrophysics, 559. doi:10.1051/0004-6361/201322515
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      Rivinius T, Baade D, Townsend RHD, Carciofi AC, Stefl S. Variable rotational line broadening in the Be star Achernar [Internet]. Astronomy & Astrophysics. 2013 ; 559[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201322515
    • Vancouver

      Rivinius T, Baade D, Townsend RHD, Carciofi AC, Stefl S. Variable rotational line broadening in the Be star Achernar [Internet]. Astronomy & Astrophysics. 2013 ; 559[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201322515
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: AGLOMERADOS DE GALÁXIAS, PERDA DE MASSA, CENTRO GALÁCTICO, GALÁXIA (VIA LÁCTEA)

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      MINNITI, D et al. Discovery of VVV CL001: a low mass globular cluster next to UKS1 in the direction of the Galactic bulge. Astronomy & Astrophysics, v. 527, p. A81/1-A81/4, 2011Tradução . . Acesso em: 24 ago. 2024.
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      Minniti, D., Hempel, M., Toledo, I., Ivanov, V. D., Alonso-García, J., Saito, R. K., et al. (2011). Discovery of VVV CL001: a low mass globular cluster next to UKS1 in the direction of the Galactic bulge. Astronomy & Astrophysics, 527, A81/1-A81/4.
    • NLM

      Minniti D, Hempel M, Toledo I, Ivanov VD, Alonso-García J, Saito RK, Catelan M, Geisler D, Jordán A, Borissova J, Zoccali M, Kurtev R, Carraro G, Barbuy BLS, Clariá J, Rejkuba M, Emerson J, Moni Bidin C. Discovery of VVV CL001: a low mass globular cluster next to UKS1 in the direction of the Galactic bulge. Astronomy & Astrophysics. 2011 ; 527 A81/1-A81/4.[citado 2024 ago. 24 ]
    • Vancouver

      Minniti D, Hempel M, Toledo I, Ivanov VD, Alonso-García J, Saito RK, Catelan M, Geisler D, Jordán A, Borissova J, Zoccali M, Kurtev R, Carraro G, Barbuy BLS, Clariá J, Rejkuba M, Emerson J, Moni Bidin C. Discovery of VVV CL001: a low mass globular cluster next to UKS1 in the direction of the Galactic bulge. Astronomy & Astrophysics. 2011 ; 527 A81/1-A81/4.[citado 2024 ago. 24 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ESTRELAS (PARÂMETROS), ASTROFÍSICA ESTELAR

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      CASAGRANDE, L et al. New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): improved astrophysical parameters for the Geneva-Copenhagen survey. Astronomy & Astrophysics, v. 530, p. A138/1-A138/21, 2011Tradução . . Acesso em: 24 ago. 2024.
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      Casagrande, L., Schönrich, R., Asplund, M., Cassisi, S., Ramírez, I., Moreno, J. L. M., et al. (2011). New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): improved astrophysical parameters for the Geneva-Copenhagen survey. Astronomy & Astrophysics, 530, A138/1-A138/21.
    • NLM

      Casagrande L, Schönrich R, Asplund M, Cassisi S, Ramírez I, Moreno JLM, Bensby T, Feltzing S. New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): improved astrophysical parameters for the Geneva-Copenhagen survey. Astronomy & Astrophysics. 2011 ; 530 A138/1-A138/21.[citado 2024 ago. 24 ]
    • Vancouver

      Casagrande L, Schönrich R, Asplund M, Cassisi S, Ramírez I, Moreno JLM, Bensby T, Feltzing S. New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s): improved astrophysical parameters for the Geneva-Copenhagen survey. Astronomy & Astrophysics. 2011 ; 530 A138/1-A138/21.[citado 2024 ago. 24 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA, ABUNDÂNCIA ESTELAR, GALÁXIAS

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      BARBUY, Beatriz Leonor Silveira et al. First stars: XV. Third-peak r-process element and actinide abundances in the uranium-rich star CS31082-001. Astronomy & Astrophysics, v. 534, p. A60/1-A60/12, 2011Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201117450. Acesso em: 24 ago. 2024.
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      Barbuy, B. L. S., Spite, M., Hill, V., Primas, F., Plez, B., Cayrel, R., et al. (2011). First stars: XV. Third-peak r-process element and actinide abundances in the uranium-rich star CS31082-001. Astronomy & Astrophysics, 534, A60/1-A60/12. doi:10.1051/0004-6361/201117450
    • NLM

      Barbuy BLS, Spite M, Hill V, Primas F, Plez B, Cayrel R, Spite F, Wanajo S, Mello Júnior CS, Andersen J, Nordström B, Beers TC, Bonifacio P, François P, Molaro P. First stars: XV. Third-peak r-process element and actinide abundances in the uranium-rich star CS31082-001 [Internet]. Astronomy & Astrophysics. 2011 ; 534 A60/1-A60/12.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201117450
    • Vancouver

      Barbuy BLS, Spite M, Hill V, Primas F, Plez B, Cayrel R, Spite F, Wanajo S, Mello Júnior CS, Andersen J, Nordström B, Beers TC, Bonifacio P, François P, Molaro P. First stars: XV. Third-peak r-process element and actinide abundances in the uranium-rich star CS31082-001 [Internet]. Astronomy & Astrophysics. 2011 ; 534 A60/1-A60/12.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361/201117450
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, GALÁXIA (VIA LÁCTEA), CENTRO GALÁCTICO

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      ORTOLANI, Sérgio et al. A fossil bulge globular cluster revealed by very large telescope multi-conjugate adaptative optics. The Astrophysical Journal, v. 737, p. 31/1-31/9, 2011Tradução . . Acesso em: 24 ago. 2024.
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      Ortolani, S., Barbuy, B. L. S., Momany, Y., Saviane, I., Bica, E., Jilkova, L., et al. (2011). A fossil bulge globular cluster revealed by very large telescope multi-conjugate adaptative optics. The Astrophysical Journal, 737, 31/1-31/9.
    • NLM

      Ortolani S, Barbuy BLS, Momany Y, Saviane I, Bica E, Jilkova L, Salerno GM, Jungwiert B. A fossil bulge globular cluster revealed by very large telescope multi-conjugate adaptative optics. The Astrophysical Journal. 2011 ; 737 31/1-31/9.[citado 2024 ago. 24 ]
    • Vancouver

      Ortolani S, Barbuy BLS, Momany Y, Saviane I, Bica E, Jilkova L, Salerno GM, Jungwiert B. A fossil bulge globular cluster revealed by very large telescope multi-conjugate adaptative optics. The Astrophysical Journal. 2011 ; 737 31/1-31/9.[citado 2024 ago. 24 ]
  • Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG

    Assunto: GALÁXIAS

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      ROCHA, C Da e ZIEGLER, B. L e MENDES DE OLIVEIRA, Cláudia. Intragroup diffuse light in compact groups of galaxies: II. HCG 15, 35 and 51. Monthly Notices of the Royal Astronomical Society, v. 388, n. 3, p. 1433-1443, 2008Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2008.13500.x. Acesso em: 24 ago. 2024.
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      Rocha, C. D., Ziegler, B. L., & Mendes de Oliveira, C. (2008). Intragroup diffuse light in compact groups of galaxies: II. HCG 15, 35 and 51. Monthly Notices of the Royal Astronomical Society, 388( 3), 1433-1443. doi:10.1111/j.1365-2966.2008.13500.x
    • NLM

      Rocha CD, Ziegler BL, Mendes de Oliveira C. Intragroup diffuse light in compact groups of galaxies: II. HCG 15, 35 and 51 [Internet]. Monthly Notices of the Royal Astronomical Society. 2008 ; 388( 3): 1433-1443.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1111/j.1365-2966.2008.13500.x
    • Vancouver

      Rocha CD, Ziegler BL, Mendes de Oliveira C. Intragroup diffuse light in compact groups of galaxies: II. HCG 15, 35 and 51 [Internet]. Monthly Notices of the Royal Astronomical Society. 2008 ; 388( 3): 1433-1443.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1111/j.1365-2966.2008.13500.x
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, GALÁXIAS

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      BONIFÁCIO, P et al. First stars VII - Lithium in extremely metal poor dwarfs. Astronomy and Astrophysics, v. 462, n. 3, p. 851-864, 2007Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20064834. Acesso em: 24 ago. 2024.
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      Bonifácio, P., Barbuy, B. L. S., Molaro, P., Sivarani, T., Cayrel, R., Plez, B., et al. (2007). First stars VII - Lithium in extremely metal poor dwarfs. Astronomy and Astrophysics, 462( 3), 851-864. doi:10.1051/0004-6361:20064834
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      Bonifácio P, Barbuy BLS, Molaro P, Sivarani T, Cayrel R, Plez B, Andersen J, Beers TC, Depagne E, Hill V, Nordström B, François P, Primas F. First stars VII - Lithium in extremely metal poor dwarfs [Internet]. Astronomy and Astrophysics. 2007 ;462( 3): 851-864.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361:20064834
    • Vancouver

      Bonifácio P, Barbuy BLS, Molaro P, Sivarani T, Cayrel R, Plez B, Andersen J, Beers TC, Depagne E, Hill V, Nordström B, François P, Primas F. First stars VII - Lithium in extremely metal poor dwarfs [Internet]. Astronomy and Astrophysics. 2007 ;462( 3): 851-864.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361:20064834
  • 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: 24 ago. 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 ago. 24 ]
    • 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 ago. 24 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS, ESTRELAS

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      SPITE, M et al. First stars IX - Mixing in extremely metal-poor giants. Variation of the 'ANTPOT.12 C'/'ANTPOT.13 C', [Na/Mg] and [AI/Mg] ratios. Astronomy and Astrophysics, v. 455, p. 291-301, 2006Tradução . . Acesso em: 24 ago. 2024.
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      Spite, M., Cayrel, R., Hill, V., Spite, F., François, P., Plez, B., et al. (2006). First stars IX - Mixing in extremely metal-poor giants. Variation of the 'ANTPOT.12 C'/'ANTPOT.13 C', [Na/Mg] and [AI/Mg] ratios. Astronomy and Astrophysics, 455, 291-301.
    • NLM

      Spite M, Cayrel R, Hill V, Spite F, François P, Plez B, Bonifacio P, Molaro P, Depagne E, Andersen J, Barbuy BLS, Beers TC, Nordström B, Primas F. First stars IX - Mixing in extremely metal-poor giants. Variation of the 'ANTPOT.12 C'/'ANTPOT.13 C', [Na/Mg] and [AI/Mg] ratios. Astronomy and Astrophysics. 2006 ; 455 291-301.[citado 2024 ago. 24 ]
    • Vancouver

      Spite M, Cayrel R, Hill V, Spite F, François P, Plez B, Bonifacio P, Molaro P, Depagne E, Andersen J, Barbuy BLS, Beers TC, Nordström B, Primas F. First stars IX - Mixing in extremely metal-poor giants. Variation of the 'ANTPOT.12 C'/'ANTPOT.13 C', [Na/Mg] and [AI/Mg] ratios. Astronomy and Astrophysics. 2006 ; 455 291-301.[citado 2024 ago. 24 ]
  • 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: 24 ago. 2024.
    • APA

      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 ago. 24 ] 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 ago. 24 ] 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: 24 ago. 2024.
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      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 ago. 24 ] 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 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361:20041634
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, MEIO INTERESTELAR

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      CHESNEAU, O et al. First VLTI/MIDI observations of a Be star: alpha Arae. Astronomy and Astrophysics, v. 435, p. 275-287, 2005Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20041954. Acesso em: 24 ago. 2024.
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      Chesneau, O., Meilland, A., Rivinius, T., Stee, P., Jankov, S., Souza, A. D. de, et al. (2005). First VLTI/MIDI observations of a Be star: alpha Arae. Astronomy and Astrophysics, 435, 275-287. doi:10.1051/0004-6361:20041954
    • NLM

      Chesneau O, Meilland A, Rivinius T, Stee P, Jankov S, Souza AD de, Graser U, Pacheco EJ, Kochler R, Leinert C, Morel S, Paresce F, Richichi A, Robbe-Dubois S. First VLTI/MIDI observations of a Be star: alpha Arae [Internet]. Astronomy and Astrophysics. 2005 ; 435 275-287.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361:20041954
    • Vancouver

      Chesneau O, Meilland A, Rivinius T, Stee P, Jankov S, Souza AD de, Graser U, Pacheco EJ, Kochler R, Leinert C, Morel S, Paresce F, Richichi A, Robbe-Dubois S. First VLTI/MIDI observations of a Be star: alpha Arae [Internet]. Astronomy and Astrophysics. 2005 ; 435 275-287.[citado 2024 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361:20041954
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR

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      SPITE, M et al. First stars VI-abundances of 'C', 'N', 'O', 'Li', and mixing in extremely metal-poor giants. galactic evolution of the light elements. Astronomy and Astrophysics, v. 430, p. 655-668, 2005Tradução . . Acesso em: 24 ago. 2024.
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      Spite, M., Cayrel, R., Plez, B., Hill, V., Spite, F., Depagne, E., et al. (2005). First stars VI-abundances of 'C', 'N', 'O', 'Li', and mixing in extremely metal-poor giants. galactic evolution of the light elements. Astronomy and Astrophysics, 430, 655-668.
    • NLM

      Spite M, Cayrel R, Plez B, Hill V, Spite F, Depagne E, François P, Bonifacio P, Barbuy BLS, Beers T, Andersen J, Molaro P, Nordström B, Primas F. First stars VI-abundances of 'C', 'N', 'O', 'Li', and mixing in extremely metal-poor giants. galactic evolution of the light elements. Astronomy and Astrophysics. 2005 ; 430 655-668.[citado 2024 ago. 24 ]
    • Vancouver

      Spite M, Cayrel R, Plez B, Hill V, Spite F, Depagne E, François P, Bonifacio P, Barbuy BLS, Beers T, Andersen J, Molaro P, Nordström B, Primas F. First stars VI-abundances of 'C', 'N', 'O', 'Li', and mixing in extremely metal-poor giants. galactic evolution of the light elements. Astronomy and Astrophysics. 2005 ; 430 655-668.[citado 2024 ago. 24 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: GALÁXIAS

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    • ABNT

      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: 24 ago. 2024.
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      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 ago. 24 ] 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 ago. 24 ] Available from: https://doi.org/10.1051/0004-6361:20030944

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