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Paper: Discussion Session: Formation of Disks around Be and B[e] Stars: a Common Mechanism?
Volume: 355, Stars With the B[e] Phenomenon
Page: 253
Authors: Stee, Ph.
Abstract: This is the summary of the discussion on the formation of disks around Be and B[e] stars with the aim to isolate a common mechanism. The role of the rotation versus the bi-stability hypothesis is debated with the fact that the disk may be in contact or not with the central star. The possibility of having a dense but mostly neutral equatorial region is also discussed as well as the role of the magnetic field, the binarity and the variability of B[e] disks.
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