A method for the study of accretion disk emission in cataclysmic variables: I. The model (2011)
Source: The Astrophysical Journal. Unidade: IAG
Subjects: DISCOS DE ACRESÇÃO, ESTRELAS, PERDA DE MASSA, RADIAÇÃO ULTRAVIOLETA
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PUEBLA, Raúl E et al. A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal, v. 736, p. 17/1-17/18, 2011Tradução . . Acesso em: 17 out. 2024.APA
Puebla, R. E., Diaz, M. P., Hillier, D. J., & Hubeny, I. (2011). A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal, 736, 17/1-17/18.NLM
Puebla RE, Diaz MP, Hillier DJ, Hubeny I. A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal. 2011 ; 736 17/1-17/18.[citado 2024 out. 17 ]Vancouver
Puebla RE, Diaz MP, Hillier DJ, Hubeny I. A method for the study of accretion disk emission in cataclysmic variables: I. The model. The Astrophysical Journal. 2011 ; 736 17/1-17/18.[citado 2024 out. 17 ]
