Chemical abundances in 12 red giants of the large magellanic cloud from high-resolution infrared spectroscopy (2002)
- Authors:
- Autor USP: BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v.124, p. 3241-3254, 2002
-
ABNT
SMITH, Verne V; HINKLE, Kenneth H; CUNHA, Katia; et al. Chemical abundances in 12 red giants of the large magellanic cloud from high-resolution infrared spectroscopy. Astronomical Journal, Albany, v. 124, p. 3241-3254, 2002. -
APA
Smith, V. V., Hinkle, K. H., Cunha, K., Plez, B., Labert, D. L., Pilachowski, C. A., et al. (2002). Chemical abundances in 12 red giants of the large magellanic cloud from high-resolution infrared spectroscopy. Astronomical Journal, 124, 3241-3254. -
NLM
Smith VV, Hinkle KH, Cunha K, Plez B, Labert DL, Pilachowski CA, Barbuy BLS, Melendez J, Balachandran S, Bessell M, Geisler DP, Hesser JE, Winge C. Chemical abundances in 12 red giants of the large magellanic cloud from high-resolution infrared spectroscopy. Astronomical Journal. 2002 ;124 3241-3254. -
Vancouver
Smith VV, Hinkle KH, Cunha K, Plez B, Labert DL, Pilachowski CA, Barbuy BLS, Melendez J, Balachandran S, Bessell M, Geisler DP, Hesser JE, Winge C. Chemical abundances in 12 red giants of the large magellanic cloud from high-resolution infrared spectroscopy. Astronomical Journal. 2002 ;124 3241-3254. - Chemical evolution of the galactic bulge
- Joint Discussion 1: abundance ratios in the oldest stars
- Uma base de dados atômicos e moleculares na região de `lâmbda'3000-4000 angstron
- Alpha & heavy elements abundances of nearby bulgelike dwarf stars
- Who´s who among barium stars
- Oxygem abundances in metal-poor stars from IR OH lines
- Abundâncias de oxigênio em estrelas pobres em metais
- Biblioteca de espectros sintéticos de estrelas frias para uso no estudo de populações estelares
- The galactic bulge
- New eyes on the first stars: the old bulge component and the important role of PNe in this context
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