ReP USP - Resultado da busca

Trabalho de evento-anais periodico
Signatures of an intermediate-age metal-rich bulge population (2012)
Bensby, T; Feltzing , S.; Gould, A; Johnson, J. A; Asplund, M; Adén, D; Moreno, Jorge Luiz Meléndez; Cohen, J. G; Thompson, I; Lucatello, S; Gal-Yam, A
Source: ASP Conference Series. Conference titles: Subaru International Conference. Unidade: IAG
Subjects: ESTRELAS, ASTROFÍSICA ESTELAR
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ABNT
BENSBY, T et al. Signatures of an intermediate-age metal-rich bulge population. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 03 jul. 2024. , 2012
APA
Bensby, T., Feltzing , S., Gould, A., Johnson, J. A., Asplund, M., Adén, D., et al. (2012). Signatures of an intermediate-age metal-rich bulge population. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo.
NLM
Bensby T, Feltzing S, Gould A, Johnson JA, Asplund M, Adén D, Moreno JLM, Cohen JG, Thompson I, Lucatello S, Gal-Yam A. Signatures of an intermediate-age metal-rich bulge population. ASP Conference Series. 2012 ; 458 203-204.[citado 2024 jul. 03 ]
Vancouver
Bensby T, Feltzing S, Gould A, Johnson JA, Asplund M, Adén D, Moreno JLM, Cohen JG, Thompson I, Lucatello S, Gal-Yam A. Signatures of an intermediate-age metal-rich bulge population. ASP Conference Series. 2012 ; 458 203-204.[citado 2024 jul. 03 ]
Artigo de periodico
Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars (2011)
Bensby, T; Adén, D; Moreno, Jorge Luiz Meléndez; Gould, A; Feltzing, S; Asplund, M; Johnson, J. A; Lucatello, S; Yee, J. C; Ramírez, I; Cohen, J. G; Thompson, I; Bond, I. A; Gal-Yam, A; Han, C; Sumi, T; Suzuki, D; Wada, K; Miyake, N; Furusawa, K; Ohmori, k; Saito, To; Tristram, P; Bennett, D
Source: Astronomy & Astrophysics. Unidade: IAG
Subjects: LENTES GRAVITACIONAIS, FORMAÇÃO E EVOLUÇÃO DA GALÁXIA, ABUNDÂNCIA ESTELAR
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ABNT
BENSBY, T et al. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. Astronomy & Astrophysics, v. 533, p. A134/1-A134/20, 2011Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201730560. Acesso em: 03 jul. 2024.
APA
Bensby, T., Adén, D., Moreno, J. L. M., Gould, A., Feltzing, S., Asplund, M., et al. (2011). Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. Astronomy & Astrophysics, 533, A134/1-A134/20. doi:10.1051/0004-6361/201730560
NLM
Bensby T, Adén D, Moreno JLM, Gould A, Feltzing S, Asplund M, Johnson JA, Lucatello S, Yee JC, Ramírez I, Cohen JG, Thompson I, Bond IA, Gal-Yam A, Han C, Sumi T, Suzuki D, Wada K, Miyake N, Furusawa K, Ohmori k, Saito T, Tristram P, Bennett D. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars [Internet]. Astronomy & Astrophysics. 2011 ; 533 A134/1-A134/20.[citado 2024 jul. 03 ] Available from: https://doi.org/10.1051/0004-6361/201730560
Vancouver
Bensby T, Adén D, Moreno JLM, Gould A, Feltzing S, Asplund M, Johnson JA, Lucatello S, Yee JC, Ramírez I, Cohen JG, Thompson I, Bond IA, Gal-Yam A, Han C, Sumi T, Suzuki D, Wada K, Miyake N, Furusawa K, Ohmori k, Saito T, Tristram P, Bennett D. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars [Internet]. Astronomy & Astrophysics. 2011 ; 533 A134/1-A134/20.[citado 2024 jul. 03 ] Available from: https://doi.org/10.1051/0004-6361/201730560
Trabalho de evento
Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS (2010)
Kennedy, Catherine R; Sivarani, Thirupathi; Beers Thimothy C; Rossi, Silvia Cristina Fernandes; Placco, Vinicius M; Johnson, J; Masseron, T
Source: Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Conference titles: IAU Symposium. Unidade: IAG
Subjects: ABUNDÂNCIA ESTELAR, GALÁXIAS, CARBONO
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ABNT
KENNEDY, Catherine R et al. Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. 2010, Anais.. Cambridge: Cambridge University Press, 2010. . Acesso em: 03 jul. 2024.
APA
Kennedy, C. R., Sivarani, T., Beers Thimothy C,, Rossi, S. C. F., Placco, V. M., Johnson, J., & Masseron, T. (2010). Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. In Chemical abundances in the Universe : connecting first stars to planets. Proceedings. Cambridge: Cambridge University Press.
NLM
Kennedy CR, Sivarani T, Beers Thimothy C, Rossi SCF, Placco VM, Johnson J, Masseron T. Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 jul. 03 ]
Vancouver
Kennedy CR, Sivarani T, Beers Thimothy C, Rossi SCF, Placco VM, Johnson J, Masseron T. Near-IR spectroscopy of CEMP stars with SOAR/OSIRIS. Chemical abundances in the Universe : connecting first stars to planets. Proceedings. 2010 ;[citado 2024 jul. 03 ]
Artigo de periodico
Automated determination of [Fe/H] and [C/Fe] from low-resolution spectroscopy (2009)
Marsteller, Brian; Beers, Timothy C; Thirupathi, Sivarani; Rossi, Sílvia Cristina Fernandes; Placco, Vinicius; Knapp, Gillian R; Johnson, Jennifer A; Lucatello, Sara
Source: The Astronomical Journal. Unidade: IAG
Subjects: GALÁXIAS, ABUNDÂNCIAS (ASTRONOMIA), POPULAÇÕES ESTELARES, ESPECTROSCOPIA
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ABNT
MARSTELLER, Brian et al. Automated determination of [Fe/H] and [C/Fe] from low-resolution spectroscopy. The Astronomical Journal, v. 138, p. 533-539, 2009Tradução . . Acesso em: 03 jul. 2024.
APA
Marsteller, B., Beers, T. C., Thirupathi, S., Rossi, S. C. F., Placco, V., Knapp, G. R., et al. (2009). Automated determination of [Fe/H] and [C/Fe] from low-resolution spectroscopy. The Astronomical Journal, 138, 533-539.
NLM
Marsteller B, Beers TC, Thirupathi S, Rossi SCF, Placco V, Knapp GR, Johnson JA, Lucatello S. Automated determination of [Fe/H] and [C/Fe] from low-resolution spectroscopy. The Astronomical Journal. 2009 ; 138 533-539.[citado 2024 jul. 03 ]
Vancouver
Marsteller B, Beers TC, Thirupathi S, Rossi SCF, Placco V, Knapp GR, Johnson JA, Lucatello S. Automated determination of [Fe/H] and [C/Fe] from low-resolution spectroscopy. The Astronomical Journal. 2009 ; 138 533-539.[citado 2024 jul. 03 ]
Artigo de periodico
An accelerating cosmology without dark energy (2009)
Steigman, G; Lima,José Ademir Sales de; Santos, R.C
Source: Journal of Cosmology and Astroparticle Physics. Unidade: IAG
Subjects: COSMOLOGIA, MATÉRIA ESCURA
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ABNT
STEIGMAN, G e LIMA, José Ademir Sales de e SANTOS, R.C. An accelerating cosmology without dark energy. Journal of Cosmology and Astroparticle Physics, n. 6, p. 033/1-033/17, 2009Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2009/06/033. Acesso em: 03 jul. 2024.
APA
Steigman, G., Lima, J. A. S. de, & Santos, R. C. (2009). An accelerating cosmology without dark energy. Journal of Cosmology and Astroparticle Physics, (6), 033/1-033/17. doi:10.1088/1475-7516/2009/06/033
NLM
Steigman G, Lima JAS de, Santos RC. An accelerating cosmology without dark energy [Internet]. Journal of Cosmology and Astroparticle Physics. 2009 ;(6): 033/1-033/17.[citado 2024 jul. 03 ] Available from: https://doi.org/10.1088/1475-7516/2009/06/033
Vancouver
Steigman G, Lima JAS de, Santos RC. An accelerating cosmology without dark energy [Internet]. Journal of Cosmology and Astroparticle Physics. 2009 ;(6): 033/1-033/17.[citado 2024 jul. 03 ] Available from: https://doi.org/10.1088/1475-7516/2009/06/033

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