On the CQE phase signature feature in high-resolution spectro-interferometry of Be stars (2012)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Subjects: ESTRELAS; INTERFEROMETRIA
- Language: Inglês
- Imprenta:
- Publisher place: San Francisco
- Date published: 2012
- Source:
- Título: ASP Conference Series
- Volume/Número/Paginação/Ano: v. 464, p. 141-148, 2012
- Conference titles: Conference on Circumstellar Dynamics at High Resolution
-
ABNT
FAES, D. M et al. On the CQE phase signature feature in high-resolution spectro-interferometry of Be stars. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. . Acesso em: 10 nov. 2025. , 2012 -
APA
Faes, D. M., Carciofi, A. C., Rivinius, T., Stefl, S., Baade, D., & Domiciano de Souza, A. (2012). On the CQE phase signature feature in high-resolution spectro-interferometry of Be stars. ASP Conference Series. San Francisco: Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo. -
NLM
Faes DM, Carciofi AC, Rivinius T, Stefl S, Baade D, Domiciano de Souza A. On the CQE phase signature feature in high-resolution spectro-interferometry of Be stars. ASP Conference Series. 2012 ; 464 141-148.[citado 2025 nov. 10 ] -
Vancouver
Faes DM, Carciofi AC, Rivinius T, Stefl S, Baade D, Domiciano de Souza A. On the CQE phase signature feature in high-resolution spectro-interferometry of Be stars. ASP Conference Series. 2012 ; 464 141-148.[citado 2025 nov. 10 ] - 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★,★★
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
