Fonte: Astronomy & Astrophysics. Unidade: IAG
Assuntos: MÉTODOS NUMÉRICOS, TRANSFERÊNCIA RADIATIVA, ESTRELAS, CINEMÁTICA, DINÂMICA
ABNT
ESCOLANO, C et al. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis. Astronomy & Astrophysics, v. 576, p. A112/1-A112/15, 2015Tradução . . Disponível em: https://doi.org/10.1051/0004-6361/201425446. Acesso em: 21 ago. 2024.APA
Escolano, C., Carciofi, A. C., Okazaki, A. T., Rivinius, T., Baade, D., & Štefl, S. (2015). 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis. Astronomy & Astrophysics, 576, A112/1-A112/15. doi:10.1051/0004-6361/201425446NLM
Escolano C, Carciofi AC, Okazaki AT, Rivinius T, Baade D, Štefl S. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis [Internet]. Astronomy & Astrophysics. 2015 ; 576 A112/1-A112/15.[citado 2024 ago. 21 ] Available from: https://doi.org/10.1051/0004-6361/201425446Vancouver
Escolano C, Carciofi AC, Okazaki AT, Rivinius T, Baade D, Štefl S. 2.5D global-disk oscillation models of the Be shell star 'dzeta' Tauri: I. Spectroscopic and polarimetric analysis [Internet]. Astronomy & Astrophysics. 2015 ; 576 A112/1-A112/15.[citado 2024 ago. 21 ] Available from: https://doi.org/10.1051/0004-6361/201425446