The Delta Scorpii Be binary: the disk development and periastron 2011 (2011)
- Authors:
- Autor USP: CARCIOFI, ALEX CAVALIERI - IAG
- Unidade: IAG
- Subjects: ESTRELAS BINÁRIAS; ESTRELAS
- Language: Inglês
- Imprenta:
- Publisher: American Astronomical Society
- Publisher place: Washington
- Date published: 2011
- Source:
- Título: AAS 217th Abstracts
- Conference titles: Meeting of the American Astronomical Society with the Historical Astronomy Division (HAD) and the High Energy Astrophysics Division (HEAD)
-
ABNT
MIROSHNICHENKO, Anatoly S et al. The Delta Scorpii Be binary: the disk development and periastron 2011. 2011, Anais.. Washington: American Astronomical Society, 2011. . Acesso em: 14 jul. 2025. -
APA
Miroshnichenko, A. S., Stefl, S., Manset, N., Bjorkman, K. S., Korpela, M., Davidson, J., et al. (2011). The Delta Scorpii Be binary: the disk development and periastron 2011. In AAS 217th Abstracts. Washington: American Astronomical Society. -
NLM
Miroshnichenko AS, Stefl S, Manset N, Bjorkman KS, Korpela M, Davidson J, Rivinius T, Okazaki AT, Carciofi AC, Pollmann E, Heathcote B, Levato H, Grosso M, Fabregat J, Zharikov SV. The Delta Scorpii Be binary: the disk development and periastron 2011. AAS 217th Abstracts. 2011 ;[citado 2025 jul. 14 ] -
Vancouver
Miroshnichenko AS, Stefl S, Manset N, Bjorkman KS, Korpela M, Davidson J, Rivinius T, Okazaki AT, Carciofi AC, Pollmann E, Heathcote B, Levato H, Grosso M, Fabregat J, Zharikov SV. The Delta Scorpii Be binary: the disk development and periastron 2011. AAS 217th Abstracts. 2011 ;[citado 2025 jul. 14 ] - Estudos das características de emissão de discos de estrelas Be
- 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★,★★
- Orbital solution leading to an acceptable interpretation for the enigmatic gamma-ray binary HESS J0632+057
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