Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood (2002)
- Authors:
- USP affiliated authors: LEPINE, JACQUES RAYMOND DANIEL - IAG ; MACIEL, WALTER JUNQUEIRA - IAG ; BARBUY, BEATRIZ LEONOR SILVEIRA - IAG
- Unidade: IAG
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v.381, p.32-50, 2002
-
ABNT
ANDRIEVSKY, A M et al. Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics, v. 381, p. 32-50, 2002Tradução . . Acesso em: 24 jan. 2026. -
APA
Andrievsky, A. M., Kovtyukh, V. V., Luck, R. E., Lépine, J. R. D., Bersier, D., Maciel, W. J., et al. (2002). Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics, 381, 32-50. -
NLM
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Bersier D, Maciel WJ, Barbuy BLS, Klochkova VG, Panchuk VE, Karpischek RU. Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics. 2002 ;381 32-50.[citado 2026 jan. 24 ] -
Vancouver
Andrievsky AM, Kovtyukh VV, Luck RE, Lépine JRD, Bersier D, Maciel WJ, Barbuy BLS, Klochkova VG, Panchuk VE, Karpischek RU. Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood. Astronomy and Astrophysics. 2002 ;381 32-50.[citado 2026 jan. 24 ] - Rotation curve of the galaxy obtained from planetary nebulae and agb stars
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