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

    Subjects: ATMOSFERAS ESTELARES, ABUNDÂNCIA ESTELAR, ESTRELAS

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      ERNANDES, H et al. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, v. 510, p. 5362-5375, 2022Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab3789. Acesso em: 17 abr. 2024.
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      Ernandes, H., Barbuy, B. L. S., Friaça, A. C. S., Hill, V., Spite, M., Spite, F., et al. (2022). Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy. Monthly Notices of the Royal Astronomical Society, 510, 5362-5375. doi:10.1093/mnras/stab3789
    • NLM

      Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1093/mnras/stab3789
    • Vancouver

      Ernandes H, Barbuy BLS, Friaça ACS, Hill V, Spite M, Spite F, Castilho BV, Evans CJ. Be, V, and Cu in the halo star CS 31082-001 from near-UV spectroscopy [Internet]. Monthly Notices of the Royal Astronomical Society. 2022 ; 510 5362-5375.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1093/mnras/stab3789
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES

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    • ABNT

      SPITE, F et al. Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars★. Astronomy & Astrophysics, v. 611, n. A30 p. 10p, 2018Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201732096. Acesso em: 17 abr. 2024.
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      Spite, F., Spite, M., Barbuy, B. L. S., Bonifacio, P., Caffau, E., & Francois, P. (2018). Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars★. Astronomy & Astrophysics, 611( A30 p. 10p). doi:10.1051/0004-6361/201732096
    • NLM

      Spite F, Spite M, Barbuy BLS, Bonifacio P, Caffau E, Francois P. Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars★ [Internet]. Astronomy & Astrophysics. 2018 ; 611( A30 p. 10p):[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201732096
    • Vancouver

      Spite F, Spite M, Barbuy BLS, Bonifacio P, Caffau E, Francois P. Abundance patterns of the light neutron-capture elements in very and extremely metal-poor stars★ [Internet]. Astronomy & Astrophysics. 2018 ; 611( A30 p. 10p):[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201732096
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES

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      SIQUEIRA MELLO, C et al. High-resolution abundance analysis of HD 140283. Astronomy & Astrophysics, v. 584, p. A86/1-A86/19, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201526695. Acesso em: 17 abr. 2024.
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      Siqueira Mello, C., Andrievsky, S. M., Barbuy, B. L. S., Spite, M., Spite, F., & Korotin, S. A. (2015). High-resolution abundance analysis of HD 140283. Astronomy & Astrophysics, 584, A86/1-A86/19. doi:10.1051/0004-6361/201526695
    • NLM

      Siqueira Mello C, Andrievsky SM, Barbuy BLS, Spite M, Spite F, Korotin SA. High-resolution abundance analysis of HD 140283 [Internet]. Astronomy & Astrophysics. 2015 ; 584 A86/1-A86/19.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201526695
    • Vancouver

      Siqueira Mello C, Andrievsky SM, Barbuy BLS, Spite M, Spite F, Korotin SA. High-resolution abundance analysis of HD 140283 [Internet]. Astronomy & Astrophysics. 2015 ; 584 A86/1-A86/19.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201526695
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIA (VIA LÁCTEA), GALÁXIAS, ABUNDÂNCIA ESTELAR

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      SIQUEIRA MELLO, C. et al. High-resolution abundance analysis of very metal-poor r-I stars. Astronomy & Astrophysics, v. 565, p. A93/1-A93/23, 2014Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201423826. Acesso em: 17 abr. 2024.
    • APA

      Siqueira Mello, C., Hill, V., Barbuy, B. L. S., Spite, M., Spite, F., Beers , T. C., et al. (2014). High-resolution abundance analysis of very metal-poor r-I stars. Astronomy & Astrophysics, 565, A93/1-A93/23. doi:10.1051/0004-6361/201423826
    • NLM

      Siqueira Mello C, Hill V, Barbuy BLS, Spite M, Spite F, Beers TC, Caffau E, Bonifacio P, Cayrel R, François P, Schatz H, Wanajo S. High-resolution abundance analysis of very metal-poor r-I stars [Internet]. Astronomy & Astrophysics. 2014 ; 565 A93/1-A93/23.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201423826
    • Vancouver

      Siqueira Mello C, Hill V, Barbuy BLS, Spite M, Spite F, Beers TC, Caffau E, Bonifacio P, Cayrel R, François P, Schatz H, Wanajo S. High-resolution abundance analysis of very metal-poor r-I stars [Internet]. Astronomy & Astrophysics. 2014 ; 565 A93/1-A93/23.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201423826
  • Source: Memorie della Società Astronomica Italiana. Unidade: IAG

    Subjects: ABUNDÂNCIA ESTELAR, ATMOSFERAS ESTELARES, POPULAÇÕES ESTELARES, GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA)

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      SIQUEIRA MELLO, C et al. r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana, v. 85, p. 232-235, 2014Tradução . . Acesso em: 17 abr. 2024.
    • APA

      Siqueira Mello, C., Barbuy, B. L. S., Spite, M., Spite, F., Caffau, E., Hill, V., et al. (2014). r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana, 85, 232-235.
    • NLM

      Siqueira Mello C, Barbuy BLS, Spite M, Spite F, Caffau E, Hill V, Wanajo S, François P, Bonifacio P, Cayrel R. r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana. 2014 ; 85 232-235.[citado 2024 abr. 17 ]
    • Vancouver

      Siqueira Mello C, Barbuy BLS, Spite M, Spite F, Caffau E, Hill V, Wanajo S, François P, Bonifacio P, Cayrel R. r-Process abundances in metal-poor Galactic halo stars. Memorie della Società Astronomica Italiana. 2014 ; 85 232-235.[citado 2024 abr. 17 ]
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ABUNDÂNCIAESTELAR, ESTRELAS

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      MELLO JR., C. Siqueira et al. Origin of the heavy elements in HD140283: measurement of europium abundance. Astronomy & Astrophysics, v. 548, p. A42/1-A42/9, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201220100. Acesso em: 17 abr. 2024.
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      Mello Jr., C. S., Barbuy, B. L. S., Spite, M., & Spite, F. (2012). Origin of the heavy elements in HD140283: measurement of europium abundance. Astronomy & Astrophysics, 548, A42/1-A42/9. doi:10.1051/0004-6361/201220100
    • NLM

      Mello Jr. CS, Barbuy BLS, Spite M, Spite F. Origin of the heavy elements in HD140283: measurement of europium abundance [Internet]. Astronomy & Astrophysics. 2012 ; 548 A42/1-A42/9.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201220100
    • Vancouver

      Mello Jr. CS, Barbuy BLS, Spite M, Spite F. Origin of the heavy elements in HD140283: measurement of europium abundance [Internet]. Astronomy & Astrophysics. 2012 ; 548 A42/1-A42/9.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201220100
  • Source: Astronomy & Astrophysics. Unidade: IAG

    Subjects: GALÁXIAS, ESTRELAS, ABUNDÂNCIA ESTELAR

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    • ABNT

      SIQUEIRA MELLO, Júnior et al. Origin of the heavy elements in HD 140283: measurement of europium abundance. Astronomy & Astrophysics, v. 548, p. A42/1-A42/9, 2012Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201220100. Acesso em: 17 abr. 2024.
    • APA

      Siqueira Mello, J., Barbuy, B. L. S., Spite, M., & Spite, F. (2012). Origin of the heavy elements in HD 140283: measurement of europium abundance. Astronomy & Astrophysics, 548, A42/1-A42/9. doi:10.1051/0004-6361/201220100
    • NLM

      Siqueira Mello J, Barbuy BLS, Spite M, Spite F. Origin of the heavy elements in HD 140283: measurement of europium abundance [Internet]. Astronomy & Astrophysics. 2012 ; 548 A42/1-A42/9.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201220100
    • Vancouver

      Siqueira Mello J, Barbuy BLS, Spite M, Spite F. Origin of the heavy elements in HD 140283: measurement of europium abundance [Internet]. Astronomy & Astrophysics. 2012 ; 548 A42/1-A42/9.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201220100
  • 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: 17 abr. 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 abr. 17 ] 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 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361/201117450
  • Unidade: IAG

    Subjects: ESTRELAS, ABUNDÂNCIA ESTELAR, POPULAÇÕES ESTELARES, VELOCIDADE

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      BONIFACIO, P et al. Extremely metal-poor turnoff stars abundances (Bonifacio+, 2009): et al. . Strasbourg: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Disponível em: http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/A+A/501/519. Acesso em: 17 abr. 2024. , 2009
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      Bonifacio, P., Spite, M., Cayrel, R., Hill, V., Spite, F., Francois, P., et al. (2009). Extremely metal-poor turnoff stars abundances (Bonifacio+, 2009): et al. Strasbourg: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. Recuperado de http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/A+A/501/519
    • NLM

      Bonifacio P, Spite M, Cayrel R, Hill V, Spite F, Francois P, Plez B, Ludwig H-G, Caffau E, Molaro P, Depagne E, Andersen J, Barbuy BLS, Beers TC, Nordström B, Primas F. Extremely metal-poor turnoff stars abundances (Bonifacio+, 2009): et al [Internet]. 2009 ;[citado 2024 abr. 17 ] Available from: http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/A+A/501/519
    • Vancouver

      Bonifacio P, Spite M, Cayrel R, Hill V, Spite F, Francois P, Plez B, Ludwig H-G, Caffau E, Molaro P, Depagne E, Andersen J, Barbuy BLS, Beers TC, Nordström B, Primas F. Extremely metal-poor turnoff stars abundances (Bonifacio+, 2009): et al [Internet]. 2009 ;[citado 2024 abr. 17 ] Available from: http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/A+A/501/519
  • Source: Astronomy & Astrophysicsm. Unidade: IAG

    Subjects: REAÇÕES NUCLEARES, ABUNDÂNCIAS (ASTRONOMIA), COSMOLOGIA, POPULAÇÕES ESTELARES

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      GONZÁLEZ HERNÁNDEZ, J. I et al. First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032. Astronomy & Astrophysicsm, v. 480, p. 233-246, 2008Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20078847. Acesso em: 17 abr. 2024.
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      González Hernández, J. I., Bonifácio, P., Ludwig, H. -G., Caffau, E., Spite, M., Spite, F., et al. (2008). First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032. Astronomy & Astrophysicsm, 480, 233-246. doi:10.1051/0004-6361:20078847
    • NLM

      González Hernández JI, Bonifácio P, Ludwig H-G, Caffau E, Spite M, Spite F, Cayrel R, Molaro P, Hill V, Francois P, Plez B, Beers TC, Sivarani T, Andersen J, Barbuy BLS, Depagne E, Nordström B, Primas F. First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032 [Internet]. Astronomy & Astrophysicsm. 2008 ; 480 233-246.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361:20078847
    • Vancouver

      González Hernández JI, Bonifácio P, Ludwig H-G, Caffau E, Spite M, Spite F, Cayrel R, Molaro P, Hill V, Francois P, Plez B, Beers TC, Sivarani T, Andersen J, Barbuy BLS, Depagne E, Nordström B, Primas F. First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032 [Internet]. Astronomy & Astrophysicsm. 2008 ; 480 233-246.[citado 2024 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361:20078847
  • 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: 17 abr. 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 abr. 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 abr. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, GALÁXIAS

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      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 abr. 2024.
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      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 abr. 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 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361:20065440
  • Source: Convention in Astrophysics : Proceedings. Conference titles: IAU Symposium. Unidade: IAG

    Subjects: ESTRELAS, METAIS, ASTROFÍSICA ESTELAR

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      SPITE, M et al. Extra-mixing extremely metal-poor red giants. 2006, Anais.. Paris: International Astronomical Union, 2006. . Acesso em: 17 abr. 2024.
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      Spite, M., Cayrel, R., Hill, V., Spite, F., Francois, P., Plez, B., et al. (2006). Extra-mixing extremely metal-poor red giants. In Convention in Astrophysics : Proceedings. Paris: International Astronomical Union.
    • NLM

      Spite M, Cayrel R, Hill V, Spite F, Francois P, Plez B, Bonifacio P, Molaro P, Depagne E, Andersen J, Barbuy BLS, Beers TC, Nordstrom B, Primas F. Extra-mixing extremely metal-poor red giants. Convention in Astrophysics : Proceedings. 2006 ;[citado 2024 abr. 17 ]
    • Vancouver

      Spite M, Cayrel R, Hill V, Spite F, Francois P, Plez B, Bonifacio P, Molaro P, Depagne E, Andersen J, Barbuy BLS, Beers TC, Nordstrom B, Primas F. Extra-mixing extremely metal-poor red giants. Convention in Astrophysics : Proceedings. 2006 ;[citado 2024 abr. 17 ]
  • 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: galatic evolution of the light elements. Astronomy and Astrophysics, p. 655-668, 2005Tradução . . Acesso em: 17 abr. 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: 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 abr. 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 abr. 17 ]
  • 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: 17 abr. 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 abr. 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 abr. 17 ]
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Subjects: ASTROFÍSICA ESTELAR, POPULAÇÕES ESTELARES

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      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 abr. 2024.
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      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 abr. 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 abr. 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 abr. 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 abr. 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 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361:20034074
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

    How to cite
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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 abr. 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 abr. 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 abr. 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 abr. 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 abr. 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 abr. 17 ] Available from: https://doi.org/10.1051/0004-6361:20030438
  • Source: Astronomy and Astrophysics. Unidade: IAG

    Assunto: ASTROFÍSICA ESTELAR

    How to cite
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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 abr. 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 abr. 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 abr. 17 ]

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