Filtros : "Spite, F" "Astronomy and Astrophysics" "IAG" Removidos: "Freitas, Edmílson Dias de" "Argentina" Limpar

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  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS, ESTRELAS

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    • ABNT

      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: 17 nov. 2024.
    • APA

      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 nov. 17 ]
    • 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 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, GALÁXIAS

    Acesso à fonteDOIHow to cite
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    • ABNT

      SIVARANI, T et al. First stars X. The nature of three unevolved carbon-enhanced metal-poor stars. Astronomy and Astrophysics, v. 459, p. 125-135, 2006Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20065440. Acesso em: 17 nov. 2024.
    • APA

      Sivarani, T., Beers, T. C., Bonifacio, P., Molaro, P., Cayrel, R., Herwig, F., et al. (2006). First stars X. The nature of three unevolved carbon-enhanced metal-poor stars. Astronomy and Astrophysics, 459, 125-135. doi:10.1051/0004-6361:20065440
    • NLM

      Sivarani T, Beers TC, Bonifacio P, Molaro P, Cayrel R, Herwig F, Spite M, Spite F, Plez B, Andersen J, Barbuy BLS, Depagne E, Hill V, François P, Nordström B, Primas F. First stars X. The nature of three unevolved carbon-enhanced metal-poor stars [Internet]. Astronomy and Astrophysics. 2006 ; 459 125-135.[citado 2024 nov. 17 ] Available from: https://doi.org/10.1051/0004-6361:20065440
    • Vancouver

      Sivarani T, Beers TC, Bonifacio P, Molaro P, Cayrel R, Herwig F, Spite M, Spite F, Plez B, Andersen J, Barbuy BLS, Depagne E, Hill V, François P, Nordström B, Primas F. First stars X. The nature of three unevolved carbon-enhanced metal-poor stars [Internet]. Astronomy and Astrophysics. 2006 ; 459 125-135.[citado 2024 nov. 17 ] Available from: https://doi.org/10.1051/0004-6361:20065440
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR

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    • ABNT

      SPITE, M et al. First stars VI-Abundances of C, N, O, Li, and mixing in extremely metal-poor giants: galatic evolution of the light elements. Astronomy and Astrophysics, p. 655-668, 2005Tradução . . Acesso em: 17 nov. 2024.
    • APA

      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: galatic evolution of the light elements. Astronomy and Astrophysics, 655-668.
    • NLM

      Spite M, Cayrel R, Plez B, Hill V, Spite F, Depagne E, Francois P, Bonifacio P, Barbuy BLS, Beers T, Andersen J, Molaro P, Norstron B, Primas F. First stars VI-Abundances of C, N, O, Li, and mixing in extremely metal-poor giants: galatic evolution of the light elements. Astronomy and Astrophysics. 2005 ; 655-668.[citado 2024 nov. 17 ]
    • Vancouver

      Spite M, Cayrel R, Plez B, Hill V, Spite F, Depagne E, Francois P, Bonifacio P, Barbuy BLS, Beers T, Andersen J, Molaro P, Norstron B, Primas F. First stars VI-Abundances of C, N, O, Li, and mixing in extremely metal-poor giants: galatic evolution of the light elements. Astronomy and Astrophysics. 2005 ; 655-668.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, EVOLUÇÃO ESTELAR

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    • ABNT

      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: 17 nov. 2024.
    • APA

      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 nov. 17 ]
    • 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 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, POPULAÇÕES ESTELARES

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: binarity and neutron capture elements. Astronomy and Astrophysics, v. 429, p. 1031-1042, 2005Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Barbuy, B. L. S., Spite, M., Spite, F., Hill, V., Cayrel, R., Plez, B., & Petitjean, P. (2005). New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: binarity and neutron capture elements. Astronomy and Astrophysics, 429, 1031-1042.
    • NLM

      Barbuy BLS, Spite M, Spite F, Hill V, Cayrel R, Plez B, Petitjean P. New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: binarity and neutron capture elements. Astronomy and Astrophysics. 2005 ; 429 1031-1042.[citado 2024 nov. 17 ]
    • Vancouver

      Barbuy BLS, Spite M, Spite F, Hill V, Cayrel R, Plez B, Petitjean P. New analysis of the two carbon-rich stars CS 22948-27 and CS 29497-34: binarity and neutron capture elements. Astronomy and Astrophysics. 2005 ; 429 1031-1042.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

    Acesso à fonteDOIHow to cite
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    • ABNT

      CAYREL, R et al. First stars V - Abundance patterns from C to Zn and supernova yields in the early galaxy*,*. Astronomy and Astrophysics, v. 416, p. 1117-1138, 2004Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20034074. Acesso em: 17 nov. 2024.
    • APA

      Cayrel, R., Depagne, E., Spite, M., Hill, V., Spite, F., François, P., et al. (2004). First stars V - Abundance patterns from C to Zn and supernova yields in the early galaxy*,*. Astronomy and Astrophysics, 416, 1117-1138. doi:10.1051/0004-6361:20034074
    • NLM

      Cayrel R, Depagne E, Spite M, Hill V, Spite F, François P, Plez B, Beers T, Primas F, Andersen J, Barbuy BLS, Bonifacio P, Molaro P, Nordström B. First stars V - Abundance patterns from C to Zn and supernova yields in the early galaxy*,* [Internet]. Astronomy and Astrophysics. 2004 ; 416 1117-1138.[citado 2024 nov. 17 ] Available from: https://doi.org/10.1051/0004-6361:20034074
    • Vancouver

      Cayrel R, Depagne E, Spite M, Hill V, Spite F, François P, Plez B, Beers T, Primas F, Andersen J, Barbuy BLS, Bonifacio P, Molaro P, Nordström B. First stars V - Abundance patterns from C to Zn and supernova yields in the early galaxy*,* [Internet]. Astronomy and Astrophysics. 2004 ; 416 1117-1138.[citado 2024 nov. 17 ] Available from: https://doi.org/10.1051/0004-6361:20034074
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      SIVARANI, T et al. First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics, v. 413, p. 1073-1085, 2004Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Sivarani, T., Bonifacio, P., Molaro, P., Cayrel, R., Spite, M., Spite, F., et al. (2004). First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics, 413, 1073-1085.
    • NLM

      Sivarani T, Bonifacio P, Molaro P, Cayrel R, Spite M, Spite F, Plez B, Andersen J, Barbuy BLS, Beers TC, Depagne E, Hill V, François P, Nordström B, Primas F. First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics. 2004 ; 413 1073-1085.[citado 2024 nov. 17 ]
    • Vancouver

      Sivarani T, Bonifacio P, Molaro P, Cayrel R, Spite M, Spite F, Plez B, Andersen J, Barbuy BLS, Beers TC, Depagne E, Hill V, François P, Nordström B, Primas F. First satrs IV. CS 29497-030: evidence for operation of the s-process at very low metallicity. Astronomy and Astrophysics. 2004 ; 413 1073-1085.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

    Acesso à fonteDOIHow to cite
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    • ABNT

      FRANÇOIS, P et al. First stars. III. A detailed elemental abundance study of four extremely metal-poor giant stars. Astronomy and Astrophysics, v. 403, p. 1105-1114, 2003Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20030438. Acesso em: 17 nov. 2024.
    • APA

      François, P., Depagne, E., Hill, V., Spite, M., Spite, F., Plez, B., et al. (2003). First stars. III. A detailed elemental abundance study of four extremely metal-poor giant stars. Astronomy and Astrophysics, 403, 1105-1114. doi:10.1051/0004-6361:20030438
    • NLM

      François P, Depagne E, Hill V, Spite M, Spite F, Plez B, Beers TC, Barbuy BLS, Cayrel R, Andersen J, Bonifacio P, Molaro P, Nordström B, Primas F. First stars. III. A detailed elemental abundance study of four extremely metal-poor giant stars [Internet]. Astronomy and Astrophysics. 2003 ;403 1105-1114.[citado 2024 nov. 17 ] Available from: https://doi.org/10.1051/0004-6361:20030438
    • Vancouver

      François P, Depagne E, Hill V, Spite M, Spite F, Plez B, Beers TC, Barbuy BLS, Cayrel R, Andersen J, Bonifacio P, Molaro P, Nordström B, Primas F. First stars. III. A detailed elemental abundance study of four extremely metal-poor giant stars [Internet]. Astronomy and Astrophysics. 2003 ;403 1105-1114.[citado 2024 nov. 17 ] Available from: https://doi.org/10.1051/0004-6361:20030438
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      DEPAGNE, E et al. First Stars II. Elemental abundances in the extremely metal-poor star CS 22949-037: A diagnostic of early massive supernovae. Astronomy and Astrophysics, v. 390, p. 187-198, 2002Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Depagne, E., ,, Hill, V., Spite, M., Spite, F., Plez, B., et al. (2002). First Stars II. Elemental abundances in the extremely metal-poor star CS 22949-037: A diagnostic of early massive supernovae. Astronomy and Astrophysics, 390, 187-198.
    • NLM

      Depagne E, , Hill V, Spite M, Spite F, Plez B, Beers TC, Barbuy BLS, Cayrel1 R, Andersen J, Bonifacio P, François P, Nordström B, Primas F. First Stars II. Elemental abundances in the extremely metal-poor star CS 22949-037: A diagnostic of early massive supernovae. Astronomy and Astrophysics. 2002 ;390 187-198.[citado 2024 nov. 17 ]
    • Vancouver

      Depagne E, , Hill V, Spite M, Spite F, Plez B, Beers TC, Barbuy BLS, Cayrel1 R, Andersen J, Bonifacio P, François P, Nordström B, Primas F. First Stars II. Elemental abundances in the extremely metal-poor star CS 22949-037: A diagnostic of early massive supernovae. Astronomy and Astrophysics. 2002 ;390 187-198.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

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    • ABNT

      HILL, V et al. First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001: Implications for the r-process site(s) and radioactive cosmochronology. Astronomy and Astrophysics, v. 387, p. 560-579, 2002Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Hill, V., Plez, B., Cayrel, R., Beers, T. C., Nordström, B., Andersen, J., et al. (2002). First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001: Implications for the r-process site(s) and radioactive cosmochronology. Astronomy and Astrophysics, 387, 560-579.
    • NLM

      Hill V, Plez B, Cayrel R, Beers TC, Nordström B, Andersen J, Spite M, Spite F, Barbuy BLS, Bonifacio P, Depagne E, François P, Primas F. First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001: Implications for the r-process site(s) and radioactive cosmochronology. Astronomy and Astrophysics. 2002 ;387 560-579.[citado 2024 nov. 17 ]
    • Vancouver

      Hill V, Plez B, Cayrel R, Beers TC, Nordström B, Andersen J, Spite M, Spite F, Barbuy BLS, Bonifacio P, Depagne E, François P, Primas F. First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001: Implications for the r-process site(s) and radioactive cosmochronology. Astronomy and Astrophysics. 2002 ;387 560-579.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR

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    • ABNT

      CASTILHO, Bruno V et al. Beryllium abundance in lithium-rich giants*. Astronomy and Astrophysics, v. 345, n. 1, p. 249-255, 1999Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Castilho, B. V., Spite, F., Barbuy, B. L. S., Spite, M., Medeiros, J. R., & Gregório-Hetem, J. (1999). Beryllium abundance in lithium-rich giants*. Astronomy and Astrophysics, 345( 1), 249-255.
    • NLM

      Castilho BV, Spite F, Barbuy BLS, Spite M, Medeiros JR, Gregório-Hetem J. Beryllium abundance in lithium-rich giants*. Astronomy and Astrophysics. 1999 ; 345( 1): 249-255.[citado 2024 nov. 17 ]
    • Vancouver

      Castilho BV, Spite F, Barbuy BLS, Spite M, Medeiros JR, Gregório-Hetem J. Beryllium abundance in lithium-rich giants*. Astronomy and Astrophysics. 1999 ; 345( 1): 249-255.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, ASTROFÍSICA ESTELAR, ESTRELAS

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    • ABNT

      BARBUY, Beatriz Leonor Silveira et al. Analysis of two CH/CN-strong very metal-poor stars. Astronomy and Astrophysics, v. 317, n. Ja 1997, p. L63-L66, 1997Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Barbuy, B. L. S., Cayrel, R., Spite, M., Beers, T. C., Spite, F., Nordstrom, B., & Nissen, P. E. (1997). Analysis of two CH/CN-strong very metal-poor stars. Astronomy and Astrophysics, 317( Ja 1997), L63-L66.
    • NLM

      Barbuy BLS, Cayrel R, Spite M, Beers TC, Spite F, Nordstrom B, Nissen PE. Analysis of two CH/CN-strong very metal-poor stars. Astronomy and Astrophysics. 1997 ; 317( Ja 1997): L63-L66.[citado 2024 nov. 17 ]
    • Vancouver

      Barbuy BLS, Cayrel R, Spite M, Beers TC, Spite F, Nordstrom B, Nissen PE. Analysis of two CH/CN-strong very metal-poor stars. Astronomy and Astrophysics. 1997 ; 317( Ja 1997): L63-L66.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTRONOMIA, GALÁXIAS, ASTROFÍSICA ESTELAR, ASTROFÍSICA

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    • ABNT

      SPITE, F e BARBUY, Beatriz Leonor Silveira e SPITE, M. Analysis of ngc 1948 f6: 4, a star in a young association of the lmc. Astronomy and Astrophysics, v. 272, n. 1, p. 116-122, 1993Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Spite, F., Barbuy, B. L. S., & Spite, M. (1993). Analysis of ngc 1948 f6: 4, a star in a young association of the lmc. Astronomy and Astrophysics, 272( 1), 116-122.
    • NLM

      Spite F, Barbuy BLS, Spite M. Analysis of ngc 1948 f6: 4, a star in a young association of the lmc. Astronomy and Astrophysics. 1993 ; 272( 1): 116-122.[citado 2024 nov. 17 ]
    • Vancouver

      Spite F, Barbuy BLS, Spite M. Analysis of ngc 1948 f6: 4, a star in a young association of the lmc. Astronomy and Astrophysics. 1993 ; 272( 1): 116-122.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTRONOMIA

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      BARBUY, Beatriz Leonor Silveira et al. Carbon and nitrogen abundances in three supergiants of the young smc globular cluster: ngc330. Astronomy and Astrophysics, v. 247, p. 15-19, 1991Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Barbuy, B. L. S., Spite, M., Spite, F., & Milone, A. (1991). Carbon and nitrogen abundances in three supergiants of the young smc globular cluster: ngc330. Astronomy and Astrophysics, 247, 15-19.
    • NLM

      Barbuy BLS, Spite M, Spite F, Milone A. Carbon and nitrogen abundances in three supergiants of the young smc globular cluster: ngc330. Astronomy and Astrophysics. 1991 ; 247 15-19.[citado 2024 nov. 17 ]
    • Vancouver

      Barbuy BLS, Spite M, Spite F, Milone A. Carbon and nitrogen abundances in three supergiants of the young smc globular cluster: ngc330. Astronomy and Astrophysics. 1991 ; 247 15-19.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTRONOMIA

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    • ABNT

      BARBUY, Beatriz Leonor Silveira e SPITE, F e SPITE, M. Magnesium isotopes in metal-poor and metal-rich stars. Astronomy and Astrophysics, v. 178, p. 199-202, 1987Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Barbuy, B. L. S., Spite, F., & Spite, M. (1987). Magnesium isotopes in metal-poor and metal-rich stars. Astronomy and Astrophysics, 178, 199-202.
    • NLM

      Barbuy BLS, Spite F, Spite M. Magnesium isotopes in metal-poor and metal-rich stars. Astronomy and Astrophysics. 1987 ; 178 199-202.[citado 2024 nov. 17 ]
    • Vancouver

      Barbuy BLS, Spite F, Spite M. Magnesium isotopes in metal-poor and metal-rich stars. Astronomy and Astrophysics. 1987 ; 178 199-202.[citado 2024 nov. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTRONOMIA

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    • ABNT

      BARBUY, Beatriz Leonor Silveira e SPITE, F e SPITE, M. Analysis of three field halo stars and the chemical evolution of the galaxy. Astronomy and Astrophysics, v. 144, n. 2, p. 343-354, 1985Tradução . . Acesso em: 17 nov. 2024.
    • APA

      Barbuy, B. L. S., Spite, F., & Spite, M. (1985). Analysis of three field halo stars and the chemical evolution of the galaxy. Astronomy and Astrophysics, 144( 2), 343-354.
    • NLM

      Barbuy BLS, Spite F, Spite M. Analysis of three field halo stars and the chemical evolution of the galaxy. Astronomy and Astrophysics. 1985 ; 144( 2): 343-354.[citado 2024 nov. 17 ]
    • Vancouver

      Barbuy BLS, Spite F, Spite M. Analysis of three field halo stars and the chemical evolution of the galaxy. Astronomy and Astrophysics. 1985 ; 144( 2): 343-354.[citado 2024 nov. 17 ]

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