Properties of the circumstellar dust in galactic FS CMa objects (2011)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- DOI: 10.1017/S1743921311010970
- Subjects: ESTRELAS; INFRAVERMELHO; 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
MIROSHNICHENKO, Anatoly S. et al. Properties of the circumstellar dust in galactic FS CMa objects. 2011, Anais.. Paris: International Astronomical Union, 2011. Disponível em: https://doi.org/10.1017/S1743921311010970. Acesso em: 10 jan. 2026. -
APA
Miroshnichenko, A. S., Gray, R. O., Bjorkman, K. S., Rudy, R. J., Lynch, D. K., & Carciofi, A. C. (2011). Properties of the circumstellar dust in galactic FS CMa objects. In Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. Paris: International Astronomical Union. doi:10.1017/S1743921311010970 -
NLM
Miroshnichenko AS, Gray RO, Bjorkman KS, Rudy RJ, Lynch DK, Carciofi AC. Properties of the circumstellar dust in galactic FS CMa objects [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2026 jan. 10 ] Available from: https://doi.org/10.1017/S1743921311010970 -
Vancouver
Miroshnichenko AS, Gray RO, Bjorkman KS, Rudy RJ, Lynch DK, Carciofi AC. Properties of the circumstellar dust in galactic FS CMa objects [Internet]. Active OB stars: structure, evolution, mass loss, and critical limits: Proceedings. 2011 ;[citado 2026 jan. 10 ] Available from: https://doi.org/10.1017/S1743921311010970 - Simulations of discrete mass loss ejections from the surface of Be stars
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- Viscous disks in Be Stars
- Outbursts and Disk Variability in Be Stars
- Monitoramento da variabilidade polarimétrica de delta Scorpii
- Pulsations and outbursts in Be stars:: small differences – big impacts
Informações sobre o DOI: 10.1017/S1743921311010970 (Fonte: oaDOI API)
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