Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: II. Testing the 2D global disk oscillation model (2009)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Subjects: ESTRELAS; POLARIZAÇÃO (ASTRONOMIA); INTERFEROMETRIA
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomy & Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v. 504, p. 915-927, 2009
-
ABNT
CARCIOFI, Alex Cavalieri et al. Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: II. Testing the 2D global disk oscillation model. Astronomy & Astrophysics, v. 504, p. 915-927, 2009Tradução . . Acesso em: 19 jun. 2025. -
APA
Carciofi, A. C., Okazaki, A. T., Le Bouquin, J. -B., Stelf, S., Rivinius, T., Baade, D., et al. (2009). Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: II. Testing the 2D global disk oscillation model. Astronomy & Astrophysics, 504, 915-927. -
NLM
Carciofi AC, Okazaki AT, Le Bouquin J-B, Stelf S, Rivinius T, Baade D, Bjorkman JE, Hummel CA. Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: II. Testing the 2D global disk oscillation model. Astronomy & Astrophysics. 2009 ; 504 915-927.[citado 2025 jun. 19 ] -
Vancouver
Carciofi AC, Okazaki AT, Le Bouquin J-B, Stelf S, Rivinius T, Baade D, Bjorkman JE, Hummel CA. Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: II. Testing the 2D global disk oscillation model. Astronomy & Astrophysics. 2009 ; 504 915-927.[citado 2025 jun. 19 ] - Estudos das características de emissão de discos de estrelas Be
- The Delta Scorpii Be binary: the disk development and periastron 2011
- Spectroscopic observations of δ Sco through the 2011 periastron passage
- Modeling the full light curve of ω CMa
- Variability of the decretion disc of Be stars in binary systems
- The 2008+ outburst of the Be star 28 CMa: a multi-instrument study
- Dynamical evolution of viscous disks around Be stars: I. Photometry
- Polarimetric observations of "sigma" Orionis E
- Report on the ESO/IAG/USP Workshop Circumstellar Dynamics at High Resolution held at Foz do Iguaçu, Paraná State, Brazil, 27 February - 2 March 2012
- Short-term variability and mass loss in Be stars: III. BRITE and SMEI satellite photometry of 28 Cygni★,★★
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