Revealing the structure of the outer disks of classical Be stars (2017)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Subjects: ASTROFÍSICA ESTELAR; DISCOS DE ACRESÇÃO
- Language: Inglês
- Imprenta:
- Publisher: Astronomical Society of the Pacific
- Publisher place: San Francico
- Date published: 2017
- Source:
- Conference titles: Proceedings of a conference held at Charles University
-
ABNT
KLEMENT, R e CARCIOFI, Alex Cavaliéri e RIVINIUS, T. Revealing the structure of the outer disks of classical Be stars. 2017, Anais.. San Francico: Astronomical Society of the Pacific, 2017. . Acesso em: 19 jan. 2026. -
APA
Klement, R., Carciofi, A. C., & Rivinius, T. (2017). Revealing the structure of the outer disks of classical Be stars. In The B[e] phenomenon: forty years of studies. San Francico: Astronomical Society of the Pacific. -
NLM
Klement R, Carciofi AC, Rivinius T. Revealing the structure of the outer disks of classical Be stars. The B[e] phenomenon: forty years of studies. 2017 ;[citado 2026 jan. 19 ] -
Vancouver
Klement R, Carciofi AC, Rivinius T. Revealing the structure of the outer disks of classical Be stars. The B[e] phenomenon: forty years of studies. 2017 ;[citado 2026 jan. 19 ] - The first determination of the viscosity parameter in the circumstellar disk of a Be star
- Outbursts and Disk Variability in Be Stars
- Pulsations and outbursts in Be stars:: small differences – big impacts
- An analysis of the V-band light curve of the Be star ω CMa with the viscous decretion disk model
- Dynamical evolution of viscous disks around Be stars: II. Polarimetry
- Differential interferometric phases at high spectral resolution as a sensitive physical diagnostic of circumstellar disks
- Viscous disks in Be Stars
- Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: II. Testing the 2D global disk oscillation model
- Cyclic variability of the circumstellar disk of the Be star 'dzeta' Tauri: I. Long-term monitoring observations
- Classical Be stars: rapidly rotating B stars with viscous Keplerian decretion disks
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