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: Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v.124, p. 3241-3254, 2002
-
ABNT
SMITH, Verne V et al. Chemical abundances in 12 red giants of the large magellanic cloud from high-resolution infrared spectroscopy. Astronomical Journal, v. 124, p. 3241-3254, 2002Tradução . . Acesso em: 06 nov. 2024. -
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.[citado 2024 nov. 06 ] -
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.[citado 2024 nov. 06 ] - O processo s e as estrelas de bário
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