Fonte: AAS 217th Abstracts. Nome do evento: Meeting of the American Astronomical Society with the Historical Astronomy Division (HAD) and the High Energy Astrophysics Division (HEAD). Unidade: IAG
Assuntos: POLARIZAÇÃO (ASTRONOMIA), DISCOS DE ACRESÇÃO
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DRAPER, Zachary H et al. Disk-loss and disk renewal phases in classical Be stars III: Modeling effects of disk structure. 2011, Anais.. Washington: American Astronomical Society, 2011. . Acesso em: 24 out. 2025.APA
Draper, Z. H., Wisniewski, J. P., Bjorkman, K. S., Haubois, X., Carciofi, A. C., Bjorkman, J. E., & Meade, M. R. (2011). Disk-loss and disk renewal phases in classical Be stars III: Modeling effects of disk structure. In AAS 217th Abstracts. Washington: American Astronomical Society.NLM
Draper ZH, Wisniewski JP, Bjorkman KS, Haubois X, Carciofi AC, Bjorkman JE, Meade MR. Disk-loss and disk renewal phases in classical Be stars III: Modeling effects of disk structure. AAS 217th Abstracts. 2011 ;[citado 2025 out. 24 ]Vancouver
Draper ZH, Wisniewski JP, Bjorkman KS, Haubois X, Carciofi AC, Bjorkman JE, Meade MR. Disk-loss and disk renewal phases in classical Be stars III: Modeling effects of disk structure. AAS 217th Abstracts. 2011 ;[citado 2025 out. 24 ]
