Filtros : "IAG" "Astrophysics and Space Science" Limpar

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  • Source: Astrophysics and Space Science. Unidade: IAG

    Assunto: SISTEMA SOLAR

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      GERBAL, D. et al. Some newly observed properties of elliptical galaxies. Astrophysics and Space Science, v. 276, p. 861-868, 2001Tradução . . Acesso em: 19 abr. 2024.
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      Gerbal, D., Capelato, H. V., Lima Neto, G. C. B., & Márquez, I. (2001). Some newly observed properties of elliptical galaxies. Astrophysics and Space Science, 276, 861-868.
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      Gerbal D, Capelato HV, Lima Neto GCB, Márquez I. Some newly observed properties of elliptical galaxies. Astrophysics and Space Science. 2001 ; 276 861-868.[citado 2024 abr. 19 ]
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      Gerbal D, Capelato HV, Lima Neto GCB, Márquez I. Some newly observed properties of elliptical galaxies. Astrophysics and Space Science. 2001 ; 276 861-868.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, MEIO INTERESTELAR

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      MACIEL, Walter Junqueira. Helium contamination from the progenitor stars of planetary nebulae: the He/H radial gradiente and the enrichment ratio. Astrophysics and Space Science, v. 277, p. 545-563, 2001Tradução . . Acesso em: 19 abr. 2024.
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      Maciel, W. J. (2001). Helium contamination from the progenitor stars of planetary nebulae: the He/H radial gradiente and the enrichment ratio. Astrophysics and Space Science, 277, 545-563.
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      Maciel WJ. Helium contamination from the progenitor stars of planetary nebulae: the He/H radial gradiente and the enrichment ratio. Astrophysics and Space Science. 2001 ; 277 545-563.[citado 2024 abr. 19 ]
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      Maciel WJ. Helium contamination from the progenitor stars of planetary nebulae: the He/H radial gradiente and the enrichment ratio. Astrophysics and Space Science. 2001 ; 277 545-563.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      IDIART, T. P. e COSTA, Roberto Dell'Aglio Dias da e FREITAS PACHECO, José Antonio. Chemical evolution of Bulges with nuclear activity. Astrophysics and Space Science, v. 265, n. 1-4, p. 391-392, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Idiart, T. P., Costa, R. D. 'A. D. da, & Freitas Pacheco, J. A. (1999). Chemical evolution of Bulges with nuclear activity. Astrophysics and Space Science, 265( 1-4), 391-392.
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      Idiart TP, Costa RD'AD da, Freitas Pacheco JA. Chemical evolution of Bulges with nuclear activity. Astrophysics and Space Science. 1999 ; 265( 1-4): 391-392.[citado 2024 abr. 19 ]
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      Idiart TP, Costa RD'AD da, Freitas Pacheco JA. Chemical evolution of Bulges with nuclear activity. Astrophysics and Space Science. 1999 ; 265( 1-4): 391-392.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR, GALÁXIAS

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      COSTA, Roberto Dell'Aglio Dias da e MACIEL, Walter Junqueira. Chemical abundances of newly discovered planetary nebulae in the galactic bulge. Astrophysics and Space Science, v. 265, n. 1-4, p. 327-329, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Costa, R. D. 'A. D. da, & Maciel, W. J. (1999). Chemical abundances of newly discovered planetary nebulae in the galactic bulge. Astrophysics and Space Science, 265( 1-4), 327-329.
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      Costa RD'AD da, Maciel WJ. Chemical abundances of newly discovered planetary nebulae in the galactic bulge. Astrophysics and Space Science. 1999 ; 265( 1-4): 327-329.[citado 2024 abr. 19 ]
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      Costa RD'AD da, Maciel WJ. Chemical abundances of newly discovered planetary nebulae in the galactic bulge. Astrophysics and Space Science. 1999 ; 265( 1-4): 327-329.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      BARBUY, Beatriz Leonor Silveira. Abundances in individual stars of the galactic bulge. Astrophysics and Space Science, v. 265, n. 1-4, p. 319-326, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Barbuy, B. L. S. (1999). Abundances in individual stars of the galactic bulge. Astrophysics and Space Science, 265( 1-4), 319-326.
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      Barbuy BLS. Abundances in individual stars of the galactic bulge. Astrophysics and Space Science. 1999 ; 265( 1-4): 319-326.[citado 2024 abr. 19 ]
    • Vancouver

      Barbuy BLS. Abundances in individual stars of the galactic bulge. Astrophysics and Space Science. 1999 ; 265( 1-4): 319-326.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA, GALÁXIAS

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      MACIEL, Walter Junqueira e QUIREZA, C. Abundance gradients in the outer galactic disk. Astrophysics and Space Science, v. 265, n. 1-4, p. 269-270, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Maciel, W. J., & Quireza, C. (1999). Abundance gradients in the outer galactic disk. Astrophysics and Space Science, 265( 1-4), 269-270.
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      Maciel WJ, Quireza C. Abundance gradients in the outer galactic disk. Astrophysics and Space Science. 1999 ; 265( 1-4): 269-270.[citado 2024 abr. 19 ]
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      Maciel WJ, Quireza C. Abundance gradients in the outer galactic disk. Astrophysics and Space Science. 1999 ; 265( 1-4): 269-270.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      ORTEGA, Wladimir Garrido e VIEIRA, Gladys Lopes e FREITAS PACHECO, José Antonio. Dynamical properties of a sample of ellipticals. Astrophysics and Space Science, v. 262, n. 3, p. 271-295, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Ortega, W. G., Vieira, G. L., & Freitas Pacheco, J. A. (1999). Dynamical properties of a sample of ellipticals. Astrophysics and Space Science, 262( 3), 271-295.
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      Ortega WG, Vieira GL, Freitas Pacheco JA. Dynamical properties of a sample of ellipticals. Astrophysics and Space Science. 1999 ; 262( 3): 271-295.[citado 2024 abr. 19 ]
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      Ortega WG, Vieira GL, Freitas Pacheco JA. Dynamical properties of a sample of ellipticals. Astrophysics and Space Science. 1999 ; 262( 3): 271-295.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      KATZ, D. et al. In Situ study of the thick disk. Preliminary results. Astrophysics and Space Science, v. 265, n. 1/4, p. 221-224, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Katz, D., Soubiran, C., Barbuy, B. L. S., Bienaymé, O., Friel, E., Cayrel, R., et al. (1999). In Situ study of the thick disk. Preliminary results. Astrophysics and Space Science, 265( 1/4), 221-224.
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      Katz D, Soubiran C, Barbuy BLS, Bienaymé O, Friel E, Cayrel R, Coupry MF, Perrin MN, Veer CV't. In Situ study of the thick disk. Preliminary results. Astrophysics and Space Science. 1999 ; 265( 1/4): 221-224.[citado 2024 abr. 19 ]
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      Katz D, Soubiran C, Barbuy BLS, Bienaymé O, Friel E, Cayrel R, Coupry MF, Perrin MN, Veer CV't. In Situ study of the thick disk. Preliminary results. Astrophysics and Space Science. 1999 ; 265( 1/4): 221-224.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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      SPITE, M. et al. Abundances in very metal-poor stars. Astrophysics and Space Science, v. 265, n. 1-4, p. 141-144, 1999Tradução . . Acesso em: 19 abr. 2024.
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      Spite, M., Spite, F., Cayrel, R., Hill, V., Nordströn, B., Barbuy, B. L. S., et al. (1999). Abundances in very metal-poor stars. Astrophysics and Space Science, 265( 1-4), 141-144.
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      Spite M, Spite F, Cayrel R, Hill V, Nordströn B, Barbuy BLS, Beers T, Nissen PE. Abundances in very metal-poor stars. Astrophysics and Space Science. 1999 ; 265( 1-4): 141-144.[citado 2024 abr. 19 ]
    • Vancouver

      Spite M, Spite F, Cayrel R, Hill V, Nordströn B, Barbuy BLS, Beers T, Nissen PE. Abundances in very metal-poor stars. Astrophysics and Space Science. 1999 ; 265( 1-4): 141-144.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Assunto: ASTRONOMIA

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      MACIEL, Walter Junqueira e CAZETTA, J O. Gravity distances of planetary nebulae. Astrophysics and Space Science, v. 249, n. 2, p. 341-352, 1997Tradução . . Acesso em: 19 abr. 2024.
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      Maciel, W. J., & Cazetta, J. O. (1997). Gravity distances of planetary nebulae. Astrophysics and Space Science, 249( 2), 341-352.
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      Maciel WJ, Cazetta JO. Gravity distances of planetary nebulae. Astrophysics and Space Science. 1997 ; 249( 2): 341-352.[citado 2024 abr. 19 ]
    • Vancouver

      Maciel WJ, Cazetta JO. Gravity distances of planetary nebulae. Astrophysics and Space Science. 1997 ; 249( 2): 341-352.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Assunto: ASTRONOMIA

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      MACIEL, Walter Junqueira. New kinematic distances of ngc 7009 and bd + 30'GRAUS'3639 from uv and radio data. Astrophysics and Space Science, v. 229, n. 2 , p. 203-13, 1995Tradução . . Acesso em: 19 abr. 2024.
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      Maciel, W. J. (1995). New kinematic distances of ngc 7009 and bd + 30'GRAUS'3639 from uv and radio data. Astrophysics and Space Science, 229( 2 ), 203-13.
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      Maciel WJ. New kinematic distances of ngc 7009 and bd + 30'GRAUS'3639 from uv and radio data. Astrophysics and Space Science. 1995 ;229( 2 ): 203-13.[citado 2024 abr. 19 ]
    • Vancouver

      Maciel WJ. New kinematic distances of ngc 7009 and bd + 30'GRAUS'3639 from uv and radio data. Astrophysics and Space Science. 1995 ;229( 2 ): 203-13.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS (CLASSIFICAÇÃO), ASTROFÍSICA ESTELAR

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      ARAUJO, F X e FREITAS PACHECO, José Antonio. Massive winds of luminous peculiar b-type stars. Astrophysics and Space Science, v. 219, n. 2, p. 267-73, 1994Tradução . . Acesso em: 19 abr. 2024.
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      Araujo, F. X., & Freitas Pacheco, J. A. (1994). Massive winds of luminous peculiar b-type stars. Astrophysics and Space Science, 219( 2), 267-73.
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      Araujo FX, Freitas Pacheco JA. Massive winds of luminous peculiar b-type stars. Astrophysics and Space Science. 1994 ; 219( 2): 267-73.[citado 2024 abr. 19 ]
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      Araujo FX, Freitas Pacheco JA. Massive winds of luminous peculiar b-type stars. Astrophysics and Space Science. 1994 ; 219( 2): 267-73.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Assunto: ASTRONOMIA

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      MACIEL, Walter Junqueira e CAZETTA, J O. H'BETA' luminosities of planetary nebula central stars. Astrophysics and Space Science, v. 222, n. 1-2, p. 147-55, 1994Tradução . . Acesso em: 19 abr. 2024.
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      Maciel, W. J., & Cazetta, J. O. (1994). H'BETA' luminosities of planetary nebula central stars. Astrophysics and Space Science, 222( 1-2), 147-55.
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      Maciel WJ, Cazetta JO. H'BETA' luminosities of planetary nebula central stars. Astrophysics and Space Science. 1994 ;222( 1-2): 147-55.[citado 2024 abr. 19 ]
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      Maciel WJ, Cazetta JO. H'BETA' luminosities of planetary nebula central stars. Astrophysics and Space Science. 1994 ;222( 1-2): 147-55.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS, ASTROFÍSICA ESTELAR

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      LÉPINE, Jacques Raymond Daniel e DUVERT, G. Are molecular clouds formed by impact of high-velocity clouds ?. Astrophysics and Space Science, v. 217, n. 1-2, p. 195-197, 1994Tradução . . Acesso em: 19 abr. 2024.
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      Lépine, J. R. D., & Duvert, G. (1994). Are molecular clouds formed by impact of high-velocity clouds ? Astrophysics and Space Science, 217( 1-2), 195-197.
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      Lépine JRD, Duvert G. Are molecular clouds formed by impact of high-velocity clouds ? Astrophysics and Space Science. 1994 ; 217( 1-2): 195-197.[citado 2024 abr. 19 ]
    • Vancouver

      Lépine JRD, Duvert G. Are molecular clouds formed by impact of high-velocity clouds ? Astrophysics and Space Science. 1994 ; 217( 1-2): 195-197.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Assunto: ASTRONOMIA

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      MACIEL, Walter Junqueira e CHIAPPINI, C. Abundances and radial gradients from disk planetary nebulae: 'HE', n, c, and 'CL'. Astrophysics and Space Science, v. 219, n. 2 , p. 231-47, 1994Tradução . . Acesso em: 19 abr. 2024.
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      Maciel, W. J., & Chiappini, C. (1994). Abundances and radial gradients from disk planetary nebulae: 'HE', n, c, and 'CL'. Astrophysics and Space Science, 219( 2 ), 231-47.
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      Maciel WJ, Chiappini C. Abundances and radial gradients from disk planetary nebulae: 'HE', n, c, and 'CL'. Astrophysics and Space Science. 1994 ;219( 2 ): 231-47.[citado 2024 abr. 19 ]
    • Vancouver

      Maciel WJ, Chiappini C. Abundances and radial gradients from disk planetary nebulae: 'HE', n, c, and 'CL'. Astrophysics and Space Science. 1994 ;219( 2 ): 231-47.[citado 2024 abr. 19 ]
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, ESTRELAS (CLASSIFICAÇÃO)

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      ROSSI, Silvia Cristina Fernandes et al. Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities. Astrophysics and Space Science, v. 213, n. 1, p. 113-119, 1994Tradução . . Disponível em: https://doi.org/10.1007/bf00627781. Acesso em: 19 abr. 2024.
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      Rossi, S. C. F., Barbuy, B. L. S., Pineau des Forets, G., & Benevides-Soares, P. (1994). Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities. Astrophysics and Space Science, 213( 1), 113-119. doi:10.1007/bf00627781
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      Rossi SCF, Barbuy BLS, Pineau des Forets G, Benevides-Soares P. Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities [Internet]. Astrophysics and Space Science. 1994 ; 213( 1): 113-119.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00627781
    • Vancouver

      Rossi SCF, Barbuy BLS, Pineau des Forets G, Benevides-Soares P. Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities [Internet]. Astrophysics and Space Science. 1994 ; 213( 1): 113-119.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00627781
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS

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      ROCHA-PINTO, H J e ARANY-PRADO, L I e MACIEL, Walter Junqueira. Model for the chemical evolution of the galaxy with refuses. Astrophysics and Space Science, v. 211, n. ja 1994, p. 241-51, 1994Tradução . . Disponível em: https://doi.org/10.1007/bf00658227. Acesso em: 19 abr. 2024.
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      Rocha-Pinto, H. J., Arany-Prado, L. I., & Maciel, W. J. (1994). Model for the chemical evolution of the galaxy with refuses. Astrophysics and Space Science, 211( ja 1994), 241-51. doi:10.1007/bf00658227
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      Rocha-Pinto HJ, Arany-Prado LI, Maciel WJ. Model for the chemical evolution of the galaxy with refuses [Internet]. Astrophysics and Space Science. 1994 ;211( ja 1994): 241-51.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00658227
    • Vancouver

      Rocha-Pinto HJ, Arany-Prado LI, Maciel WJ. Model for the chemical evolution of the galaxy with refuses [Internet]. Astrophysics and Space Science. 1994 ;211( ja 1994): 241-51.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00658227
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS, ASTROFÍSICA

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      CONTINI, M e VIEGAS, Sueli Maria Marino. Shock and photoionization models for infrared lines from active galactic nuclei. Astrophysics and Space Science, v. 205, n. 1, p. 149-154, 1993Tradução . . Disponível em: https://doi.org/10.1007/bf00657970. Acesso em: 19 abr. 2024.
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      Contini, M., & Viegas, S. M. M. (1993). Shock and photoionization models for infrared lines from active galactic nuclei. Astrophysics and Space Science, 205( 1), 149-154. doi:10.1007/bf00657970
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      Contini M, Viegas SMM. Shock and photoionization models for infrared lines from active galactic nuclei [Internet]. Astrophysics and Space Science. 1993 ; 205( 1): 149-154.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00657970
    • Vancouver

      Contini M, Viegas SMM. Shock and photoionization models for infrared lines from active galactic nuclei [Internet]. Astrophysics and Space Science. 1993 ; 205( 1): 149-154.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00657970
  • Source: Astrophysics and Space Science. Unidade: IAG

    Assunto: ASTRONOMIA

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      MACIEL, Walter Junqueira. Space distribution and metallicities of globular clusters: the distance to the galactic centre. Astrophysics and Space Science, v. 206, n. 2 , p. 285-300, 1993Tradução . . Disponível em: https://doi.org/10.1007/bf00658152. Acesso em: 19 abr. 2024.
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      Maciel, W. J. (1993). Space distribution and metallicities of globular clusters: the distance to the galactic centre. Astrophysics and Space Science, 206( 2 ), 285-300. doi:10.1007/bf00658152
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      Maciel WJ. Space distribution and metallicities of globular clusters: the distance to the galactic centre [Internet]. Astrophysics and Space Science. 1993 ;206( 2 ): 285-300.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00658152
    • Vancouver

      Maciel WJ. Space distribution and metallicities of globular clusters: the distance to the galactic centre [Internet]. Astrophysics and Space Science. 1993 ;206( 2 ): 285-300.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00658152
  • Source: Astrophysics and Space Science. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS

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      MACIEL, Walter Junqueira. Metal-poor planetary nebulae: effects of winds. Astrophysics and Space Science, v. 209, n. 1 , p. 65-70, 1993Tradução . . Disponível em: https://doi.org/10.1007/bf00666437. Acesso em: 19 abr. 2024.
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      Maciel, W. J. (1993). Metal-poor planetary nebulae: effects of winds. Astrophysics and Space Science, 209( 1 ), 65-70. doi:10.1007/bf00666437
    • NLM

      Maciel WJ. Metal-poor planetary nebulae: effects of winds [Internet]. Astrophysics and Space Science. 1993 ;209( 1 ): 65-70.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00666437
    • Vancouver

      Maciel WJ. Metal-poor planetary nebulae: effects of winds [Internet]. Astrophysics and Space Science. 1993 ;209( 1 ): 65-70.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1007/bf00666437

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