Using Cepheids to determine the galactic abundance gradient: I. the solar neighbourhood (2002)
Source: Astronomy and Astrophysics. Unidade: IAG
Assunto: ASTROFÍSICA ESTELAR
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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: 17 nov. 2024.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 2024 nov. 17 ]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 2024 nov. 17 ]
