The circumstellar environment of the FS CMa star IRAS 00470+6429 (2011)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- DOI: 10.1017/S1743921311010830
- Subjects: ESTRELAS; VENTO; POEIRA INTERESTELAR
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2011
- Source:
- Conference titles: IAU Symposium
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
CARCIOFI, Alex Cavaliéri e MIROSHNICHENKO, Anatoly S e BJORKMAN, Jon E. The circumstellar environment of the FS CMa star IRAS 00470+6429. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311010830. Acesso em: 18 jan. 2026. -
APA
Carciofi, A. C., Miroshnichenko, A. S., & Bjorkman, J. E. (2011). The circumstellar environment of the FS CMa star IRAS 00470+6429. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311010830 -
NLM
Carciofi AC, Miroshnichenko AS, Bjorkman JE. The circumstellar environment of the FS CMa star IRAS 00470+6429 [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2026 jan. 18 ] Available from: https://doi.org/10.1017/S1743921311010830 -
Vancouver
Carciofi AC, Miroshnichenko AS, Bjorkman JE. The circumstellar environment of the FS CMa star IRAS 00470+6429 [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2026 jan. 18 ] Available from: https://doi.org/10.1017/S1743921311010830 - The first determination of the viscosity parameter in the circumstellar disk of a Be star
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- 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
Informações sobre o DOI: 10.1017/S1743921311010830 (Fonte: oaDOI API)
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