3D SPH simulations show that localized, mildly super-Keplerian equatorial mass ejections with high viscosity reproduce the photometric, spectroscopic, and polarimetric signatures of Be star flicker events.
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The birth of Be star disks III. SPH models of localised mass ejections
3D SPH simulations show that localized, mildly super-Keplerian equatorial mass ejections with high viscosity reproduce the photometric, spectroscopic, and polarimetric signatures of Be star flicker events.