Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc (2002)
- Authors:
- USP affiliated authors: LEPINE, JACQUES RAYMOND DANIEL - IAG ; MACIEL, WALTER JUNQUEIRA - IAG
- Unidade: IAG
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v.392, p.491-499, 2002
-
ABNT
ANDRIEVSKY, A M et al. Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics, v. 392, p. 491-499, 2002Tradução . . Acesso em: 19 abr. 2024. -
APA
Andrievsky, A. M., Kovtyukh, V. V., Luck, R. E., Lépine, J. R. D., Maciel, W. J., & Beletsky, Y. V. (2002). Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics, 392, 491-499. -
NLM
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Maciel WJ, Beletsky YV. Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics. 2002 ;392 491-499.[citado 2024 abr. 19 ] -
Vancouver
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Maciel WJ, Beletsky YV. Using Cepheids to determine the galactic abundance gradient: III. Firt results for the outer disc. Astronomy and Astrophysics. 2002 ;392 491-499.[citado 2024 abr. 19 ] - Barium abundances in Cepheids
- A curva de rotação da galáxia e a matéria escura
- Rotation curve of the galaxy obtained from planetary nebulae and agb stars
- Using cepheids to determine the galactic abundance gradient
- Curva de rotação da galaxia obtida a partir de nebulosas planetárias e estrelas agb
- Oxygen abundance distribution in the Galactic disc
- Elemental abundances in the centre of the Galactic nuclear disc
- Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood
- Grains and the heating of hii regions
- Grains and the galactic electron temperature gradient
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