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  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: CATÁLOGOS, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), GALÁXIA (VIA LÁCTEA), ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, ESTRELAS, CARBONO, ESPECTROSCOPIA

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      BEERS, Timothy C et al. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, v. 835, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 30 set. 2024.
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      Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis. The Astrophysical Journal, 835, 81. doi:10.3847/1538-4357/835/1/81
    • NLM

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 set. 30 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
    • Vancouver

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bright metal-poor stars from the Hamburg/ESO survey: II. A Chemodynamical Analysis [Internet]. The Astrophysical Journal. 2017 ; 835 81.[citado 2024 set. 30 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
  • Source: Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR

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      BEERS, Timothy C et al. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis. Astrophysical Journal, v. 835, n. 1, p. 81, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/835/1/81. Acesso em: 30 set. 2024.
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      Beers, T. C., Placco, V. M., Carollo, D., Rossi, S. C. F., Lee, Y. S., Frebel, A., et al. (2017). Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis. Astrophysical Journal, 835( 1), 81. doi:10.3847/1538-4357/835/1/81
    • NLM

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis [Internet]. Astrophysical Journal. 2017 ;835( 1): 81.[citado 2024 set. 30 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
    • Vancouver

      Beers TC, Placco VM, Carollo D, Rossi SCF, Lee YS, Frebel A, Norris JE, Dietz S, Masseron T. Bight metal-poor stars from the Hamburg/ESO survey. II. A chemodynamical analysis [Internet]. Astrophysical Journal. 2017 ;835( 1): 81.[citado 2024 set. 30 ] Available from: https://doi.org/10.3847/1538-4357/835/1/81
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, MEIO INTERESTELAR, NUVENS DE MAGALHÃES, CAMPO MAGNÉTICO

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      GOMES, Aiara Lobo et al. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure. The Astrophysical Journal, v. 806, p. 94/1-94/19, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/806/1/94. Acesso em: 30 set. 2024.
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      Gomes, A. L., Magalhães, A. M., Pereyra, A., & Rodrigues, C. V. (2015). A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure. The Astrophysical Journal, 806, 94/1-94/19. doi:10.1088/0004-637X/806/1/94
    • NLM

      Gomes AL, Magalhães AM, Pereyra A, Rodrigues CV. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure [Internet]. The Astrophysical Journal. 2015 ; 806 94/1-94/19.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
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      Gomes AL, Magalhães AM, Pereyra A, Rodrigues CV. A new optical polarization catalog for the small Magellanic Cloud: the magnetic field structure [Internet]. The Astrophysical Journal. 2015 ; 806 94/1-94/19.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/806/1/94
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: GALÁXIAS, GALÁXIAS (EVOLUÇÃO;INTERAÇÃO), DINÂMICA DAS GALÁXIAS

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      TORRES-FLORES, S et al. Witnessing gas mixing in the metal distribution of the Hickson compact group HCG 31. The Astrophysical Journal Letters, v. 798, p. L24/1-L24/5, 2015Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/798/1/L24. Acesso em: 30 set. 2024.
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      Torres-Flores, S., Oliveira, C. L. M. de, Amram, P., Alfaro-Cuello, M., Carrasco, E. R., & Mello, D. F. de. (2015). Witnessing gas mixing in the metal distribution of the Hickson compact group HCG 31. The Astrophysical Journal Letters, 798, L24/1-L24/5. doi:10.1088/2041-8205/798/1/L24
    • NLM

      Torres-Flores S, Oliveira CLM de, Amram P, Alfaro-Cuello M, Carrasco ER, Mello DF de. Witnessing gas mixing in the metal distribution of the Hickson compact group HCG 31 [Internet]. The Astrophysical Journal Letters. 2015 ; 798 L24/1-L24/5.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/2041-8205/798/1/L24
    • Vancouver

      Torres-Flores S, Oliveira CLM de, Amram P, Alfaro-Cuello M, Carrasco ER, Mello DF de. Witnessing gas mixing in the metal distribution of the Hickson compact group HCG 31 [Internet]. The Astrophysical Journal Letters. 2015 ; 798 L24/1-L24/5.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/2041-8205/798/1/L24
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: DISCOS DE ACRESÇÃO, GALÁXIAS, GALÁXIAS SEY FERT

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      SCHIMOIA, Jaderson S et al. Short-timescale monitoring of the X-ray, UV, and broad double-peak emission line of the nucleus of NGC 1097. The Astrophysical Journal, v. 800, p. 63/1-63/13, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/800/1/63. Acesso em: 30 set. 2024.
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      Schimoia, J. S., Storchi-Bergmann, T., Grupe, D., Eracleous, M., Peterson, B. M., Baldwin, J. A., et al. (2015). Short-timescale monitoring of the X-ray, UV, and broad double-peak emission line of the nucleus of NGC 1097. The Astrophysical Journal, 800, 63/1-63/13. doi:10.1088/0004-637X/800/1/63
    • NLM

      Schimoia JS, Storchi-Bergmann T, Grupe D, Eracleous M, Peterson BM, Baldwin JA, Silva RN da, Winge C. Short-timescale monitoring of the X-ray, UV, and broad double-peak emission line of the nucleus of NGC 1097 [Internet]. The Astrophysical Journal. 2015 ; 800 63/1-63/13.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/800/1/63
    • Vancouver

      Schimoia JS, Storchi-Bergmann T, Grupe D, Eracleous M, Peterson BM, Baldwin JA, Silva RN da, Winge C. Short-timescale monitoring of the X-ray, UV, and broad double-peak emission line of the nucleus of NGC 1097 [Internet]. The Astrophysical Journal. 2015 ; 800 63/1-63/13.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/800/1/63
  • 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: 30 set. 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
    • NLM

      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 set. 30 ] 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 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/795/1/89
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: GALÁXIAS, GALÁXIAS ATIVAS, ESPECTROSCOPIA

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      MENEZES, R. B e STEINER, João Evangelista e RICCI, T. V. An off-centered active galactic nucleus in NGC 3115. The Astrophysical Journal Letters, v. 796, p. L13/1-L13/6, 2014Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/796/1/L13. Acesso em: 30 set. 2024.
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      Menezes, R. B., Steiner, J. E., & Ricci, T. V. (2014). An off-centered active galactic nucleus in NGC 3115. The Astrophysical Journal Letters, 796, L13/1-L13/6. doi:10.1088/2041-8205/796/1/L13
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      Menezes RB, Steiner JE, Ricci TV. An off-centered active galactic nucleus in NGC 3115 [Internet]. The Astrophysical Journal Letters. 2014 ; 796 L13/1-L13/6.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/2041-8205/796/1/L13
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      Menezes RB, Steiner JE, Ricci TV. An off-centered active galactic nucleus in NGC 3115 [Internet]. The Astrophysical Journal Letters. 2014 ; 796 L13/1-L13/6.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/2041-8205/796/1/L13
  • Source: AAS Meeting 223. Conference titles: Annual AAS Meeting. Unidade: IAG

    Subjects: ESTRELAS, GALÁXIAS

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      DE MELLO, Duilia F et al. Stellar clusters formed from debris of colliding galaxies. 2014, Anais.. Washington: American Astronomical Society, 2014. . Acesso em: 30 set. 2024.
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      De Mello, D. F., Oliveira, C. L. M. de, Torres-Flores, S., & Urrutia-Viscarra, F. (2014). Stellar clusters formed from debris of colliding galaxies. In AAS Meeting 223. Washington: American Astronomical Society.
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      De Mello DF, Oliveira CLM de, Torres-Flores S, Urrutia-Viscarra F. Stellar clusters formed from debris of colliding galaxies. AAS Meeting 223. 2014 ;[citado 2024 set. 30 ]
    • Vancouver

      De Mello DF, Oliveira CLM de, Torres-Flores S, Urrutia-Viscarra F. Stellar clusters formed from debris of colliding galaxies. AAS Meeting 223. 2014 ;[citado 2024 set. 30 ]
  • Source: The Astrophysical Journal Letters. Unidade: IAG

    Subjects: COSMOLOGIA (PARÂMETROS), GALÁXIAS

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      LIMA, José Ademir Sales de e CUNHA, J. V. A 3% determination of Ho at intermediate redshifts. The Astrophysical Journal Letters, v. 78, p. L38/1-L38/6, 2014Tradução . . Disponível em: https://doi.org/10.1088/2041-8205/781/2/L38. Acesso em: 30 set. 2024.
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      Lima, J. A. S. de, & Cunha, J. V. (2014). A 3% determination of Ho at intermediate redshifts. The Astrophysical Journal Letters, 78, L38/1-L38/6. doi:10.1088/2041-8205/781/2/L38
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      Lima JAS de, Cunha JV. A 3% determination of Ho at intermediate redshifts [Internet]. The Astrophysical Journal Letters. 2014 ;78 L38/1-L38/6.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/2041-8205/781/2/L38
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      Lima JAS de, Cunha JV. A 3% determination of Ho at intermediate redshifts [Internet]. The Astrophysical Journal Letters. 2014 ;78 L38/1-L38/6.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/2041-8205/781/2/L38
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, ESPECTROSCOPIA

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      PLACCO, Vinicius M et al. Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5. The Astrophysical Journal, v. 781, n. 40, p. 1-14, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/781/1/40. Acesso em: 30 set. 2024.
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      Placco, V. M., Frebel, A., Beers, T. C., Beers, T. C., Christlieb, N., Lee, Y. S., et al. (2014). Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H] <= -3,5. The Astrophysical Journal, 781( 40), 1-14. doi:10.1088/0004-637X/781/1/40
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      Placco VM, Frebel A, Beers TC, Beers TC, Christlieb N, Lee YS, Kennedy CR, Rossi SCF, Santucci RM. Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H]<= -3,5 [Internet]. The Astrophysical Journal. 2014 ; 781( 40): 1-14.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/1/40
    • Vancouver

      Placco VM, Frebel A, Beers TC, Beers TC, Christlieb N, Lee YS, Kennedy CR, Rossi SCF, Santucci RM. Metal-poor stars observed with the Magellan Telescope.: II. Discovery of four stars with [Fe/H]<= -3,5 [Internet]. The Astrophysical Journal. 2014 ; 781( 40): 1-14.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/1/40
  • Source: The Astrophysical Journal. Unidades: IAG, EACH

    Subjects: GALÁXIAS, CAMPO MAGNÉTICO, MAGNETOHIDRODINÂMICA, TURBULÊNCIA

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      SANTOS-LIMA, R et al. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium. The Astrophysical Journal, v. 781, n. 2, p. 1-21, 2014Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/781/2/84. Acesso em: 30 set. 2024.
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      Santos-Lima, R., Dal Pino, E. M. de G., Kowal, G., Falceta Gonçalves, D. A., Lazarian, A., & Nakwacki, M. S. (2014). Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium. The Astrophysical Journal, 781( 2), 1-21. doi:10.1088/0004-637X/781/2/84
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      Santos-Lima R, Dal Pino EM de G, Kowal G, Falceta Gonçalves DA, Lazarian A, Nakwacki MS. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium [Internet]. The Astrophysical Journal. 2014 ; 781( 2): 1-21.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
    • Vancouver

      Santos-Lima R, Dal Pino EM de G, Kowal G, Falceta Gonçalves DA, Lazarian A, Nakwacki MS. Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium [Internet]. The Astrophysical Journal. 2014 ; 781( 2): 1-21.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/781/2/84
  • Source: Proceedings of SPIE. Unidade: IAG

    Subjects: TELESCÓPIOS, POPULAÇÕES ESTELARES, GALÁXIAS, ESTRELAS

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      EVANS, C. J et al. Science case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large Telescope. Proceedings of SPIE. Bellingham: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Disponível em: https://doi.org/10.1117/12.2055857. Acesso em: 30 set. 2024. , 2014
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      Evans, C. J., Puech, M., Barbuy, B. L. S., & Bonifacio, P. (2014). Science case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large Telescope. Proceedings of SPIE. Bellingham: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. doi:10.1117/12.2055857
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      Evans CJ, Puech M, Barbuy BLS, Bonifacio P. Science case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large Telescope [Internet]. Proceedings of SPIE. 2014 ; 9147 914796/1-914796/17.[citado 2024 set. 30 ] Available from: https://doi.org/10.1117/12.2055857
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      Evans CJ, Puech M, Barbuy BLS, Bonifacio P. Science case and requirements for the MOSAIC concept for a multi-object spectrograph for the European Extremely Large Telescope [Internet]. Proceedings of SPIE. 2014 ; 9147 914796/1-914796/17.[citado 2024 set. 30 ] Available from: https://doi.org/10.1117/12.2055857
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, ESPECTROSCOPIA

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      PLACCO, Vinicius M et al. Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis. The Astrophysical Journal, v. 770, n. 2, p. 104/1-104/22, 2013Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/770/2/104. Acesso em: 30 set. 2024.
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      Placco, V. M., Frebel, A., Beers, T. C., Karakas, A. I., Kennedy, C. R., Rossi, S. C. F., et al. (2013). Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis. The Astrophysical Journal, 770( 2), 104/1-104/22. doi:10.1088/0004-637X/770/2/104
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      Placco VM, Frebel A, Beers TC, Karakas AI, Kennedy CR, Rossi SCF, Christlieb N, Stancliffe RJ. Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis [Internet]. The Astrophysical Journal. 2013 ; 770( 2): 104/1-104/22.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/770/2/104
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      Placco VM, Frebel A, Beers TC, Karakas AI, Kennedy CR, Rossi SCF, Christlieb N, Stancliffe RJ. Metal-poor stars observed with the Magellan Telescope: I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesis [Internet]. The Astrophysical Journal. 2013 ; 770( 2): 104/1-104/22.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/770/2/104
  • Unidade: IAG

    Subjects: NOTÍCIA, GALÁXIA (VIA LÁCTEA), LÍTIO, GALÁXIAS

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      MORENO, Jorge Luiz Meléndez. International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin]. . Mauna Kea: W. M. Keck Observatory. Disponível em: http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory. Acesso em: 30 set. 2024. , 2013
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      Moreno, J. L. M. (2013). International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin]. Mauna Kea: W. M. Keck Observatory. Recuperado de http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory
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      Moreno JLM. International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin] [Internet]. 2013 ;[citado 2024 set. 30 ] Available from: http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory
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      Moreno JLM. International team on Keck Observatory strengthens Big Bang theory. [Depoimento a Karin Lind e Davide De Martin] [Internet]. 2013 ;[citado 2024 set. 30 ] Available from: http://www.keckobservatory.org/recent/entry/international_team_on_keck_observatory_strengthens_big_bang_theory
  • Conference titles: AAS Meeting. Unidade: IAG

    Subjects: GALÁXIAS ESPIRAIS, GALÁXIAS

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      EUFRASIO, R. T et al. When the UV unveils the largest spiral. 2013, Anais.. Washington: American Astronomical Society, 2013. . Acesso em: 30 set. 2024.
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      Eufrasio, R. T., De Mello, D. F., Dwek, E., Urrutia-Viscarra, F., & Oliveira, C. L. M. de. (2013). When the UV unveils the largest spiral. In . Washington: American Astronomical Society.
    • NLM

      Eufrasio RT, De Mello DF, Dwek E, Urrutia-Viscarra F, Oliveira CLM de. When the UV unveils the largest spiral. 2013 ;[citado 2024 set. 30 ]
    • Vancouver

      Eufrasio RT, De Mello DF, Dwek E, Urrutia-Viscarra F, Oliveira CLM de. When the UV unveils the largest spiral. 2013 ;[citado 2024 set. 30 ]
  • Source: AIP Conference Proceedings. Conference titles: Conference on Cosmology and Gravitation in the Southern Cone (I Cosmo Sul). Unidade: IAG

    Subjects: GALÁXIAS, COSMOLOGIA

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      SODRÉ JÚNIOR, Laerte. Cosmology with large redshift surveys. AIP Conference Proceedings. College Park: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Disponível em: https://doi.org/10.1063/1.4756806. Acesso em: 30 set. 2024. , 2012
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      Sodré Júnior, L. (2012). Cosmology with large redshift surveys. AIP Conference Proceedings. College Park: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. doi:10.1063/1.4756806
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      Sodré Júnior L. Cosmology with large redshift surveys [Internet]. AIP Conference Proceedings. 2012 ; 1471 22-26.[citado 2024 set. 30 ] Available from: https://doi.org/10.1063/1.4756806
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      Sodré Júnior L. Cosmology with large redshift surveys [Internet]. AIP Conference Proceedings. 2012 ; 1471 22-26.[citado 2024 set. 30 ] Available from: https://doi.org/10.1063/1.4756806
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, MEIO INTERGALÁTICO, RAIOS X

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      MILLER, Eric D et al. Finding fossil groups: optical identification and X-ray confirmation. The Astrophysical Journal, v. 747, p. 94/1-94/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/747/2/94. Acesso em: 30 set. 2024.
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      Miller, E. D., Rycoff, E., Dupke, R. A., Oliveira, C. M. de, Oliveira, R. L. de, Proctor, R. N., et al. (2012). Finding fossil groups: optical identification and X-ray confirmation. The Astrophysical Journal, 747, 94/1-94/13. doi:10.1088/0004-637X/747/2/94
    • NLM

      Miller ED, Rycoff E, Dupke RA, Oliveira CM de, Oliveira RL de, Proctor RN, Garmire GP, Koester BP, McKay TA. Finding fossil groups: optical identification and X-ray confirmation [Internet]. The Astrophysical Journal. 2012 ; 747 94/1-94/13.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/747/2/94
    • Vancouver

      Miller ED, Rycoff E, Dupke RA, Oliveira CM de, Oliveira RL de, Proctor RN, Garmire GP, Koester BP, McKay TA. Finding fossil groups: optical identification and X-ray confirmation [Internet]. The Astrophysical Journal. 2012 ; 747 94/1-94/13.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/747/2/94
  • Source: The Astrophysical Journal. Unidade: IAG

    Subjects: GALÁXIAS, AGLOMERADOS DE GALÁXIAS, MEIO INTERGALÁTICO, ESTRUTURA DO UNIVERSO, RAIOS X

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      ANDRADE-SANTOS, Felipe e LIMA NETO, Gastão César Bierrenbach e LAGANÁ, Tatiana Ferraz. A new method to quantify X-ray substructures in clusters of galaxies. The Astrophysical Journal, v. 746, p. 139/1-139/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/746/2/139. Acesso em: 30 set. 2024.
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      Andrade-Santos, F., Lima Neto, G. C. B., & Laganá, T. F. (2012). A new method to quantify X-ray substructures in clusters of galaxies. The Astrophysical Journal, 746, 139/1-139/13. doi:10.1088/0004-637X/746/2/139
    • NLM

      Andrade-Santos F, Lima Neto GCB, Laganá TF. A new method to quantify X-ray substructures in clusters of galaxies [Internet]. The Astrophysical Journal. 2012 ; 746 139/1-139/13.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/746/2/139
    • Vancouver

      Andrade-Santos F, Lima Neto GCB, Laganá TF. A new method to quantify X-ray substructures in clusters of galaxies [Internet]. The Astrophysical Journal. 2012 ; 746 139/1-139/13.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-637X/746/2/139
  • Source: Proceedings of SPIE. Conference titles: Ground-based and Airborne Instrumentation for Astronomy. Unidade: IAG

    Subjects: TELESCÓPIOS, ESTRELAS, GALÁXIAS, GALÁXIAS (EVOLUÇÃO), INSTRUMENTAÇÃO (ASTRONOMIA)

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      EVANS, C. J e BARBUY, Beatriz Leonor Silveira e BONIFACIO, P. Multi-object spectroscopy with the European ELT: scientific synergies between EAGLE & EVE. 2012, Anais.. Bellingham: SPIE, 2012. Disponível em: https://doi.org/10.1117/12.924819. Acesso em: 30 set. 2024.
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      Evans, C. J., Barbuy, B. L. S., & Bonifacio, P. (2012). Multi-object spectroscopy with the European ELT: scientific synergies between EAGLE & EVE. In Proceedings of SPIE (Vol. 8446). Bellingham: SPIE. doi:10.1117/12.924819
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      Evans CJ, Barbuy BLS, Bonifacio P. Multi-object spectroscopy with the European ELT: scientific synergies between EAGLE & EVE [Internet]. Proceedings of SPIE. 2012 ; 8446[citado 2024 set. 30 ] Available from: https://doi.org/10.1117/12.924819
    • Vancouver

      Evans CJ, Barbuy BLS, Bonifacio P. Multi-object spectroscopy with the European ELT: scientific synergies between EAGLE & EVE [Internet]. Proceedings of SPIE. 2012 ; 8446[citado 2024 set. 30 ] Available from: https://doi.org/10.1117/12.924819
  • Source: The Astronomical Journal. Unidade: IAG

    Subjects: GALÁXIAS, ESTRUTURA DA GALÁXIA, MEIO INTERESTELAR

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      AMÔRES, E. B et al. Galaxies behind the galactic plane: first results and perspectives from the VVV survey. The Astronomical Journal, v. 144, p. 127/1-127/11, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-6256/144/5/127. Acesso em: 30 set. 2024.
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      Amôres, E. B., Sodré Júnior, L., Minniti, D., Alonso, M. V., Padilla, N., Gurovich, S., et al. (2012). Galaxies behind the galactic plane: first results and perspectives from the VVV survey. The Astronomical Journal, 144, 127/1-127/11. doi:10.1088/0004-6256/144/5/127
    • NLM

      Amôres EB, Sodré Júnior L, Minniti D, Alonso MV, Padilla N, Gurovich S, Arsenijevic V, Tollerud EJ, Rodríguez-Ardila A, Díaz Tello J, Lucas W. Galaxies behind the galactic plane: first results and perspectives from the VVV survey [Internet]. The Astronomical Journal. 2012 ; 144 127/1-127/11.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-6256/144/5/127
    • Vancouver

      Amôres EB, Sodré Júnior L, Minniti D, Alonso MV, Padilla N, Gurovich S, Arsenijevic V, Tollerud EJ, Rodríguez-Ardila A, Díaz Tello J, Lucas W. Galaxies behind the galactic plane: first results and perspectives from the VVV survey [Internet]. The Astronomical Journal. 2012 ; 144 127/1-127/11.[citado 2024 set. 30 ] Available from: https://doi.org/10.1088/0004-6256/144/5/127

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