Discussion Session: Formation of Disks around Be and B[e] Stars: A Common Mechanism ?

Details Discussion Session: Formation of Disks around Be and B[e] Stars: A Common Mechanism ? Discussion Session: Formation of Disks around Be and B[e] Stars: A Common Mechanism ?

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..355..253s&link_type=abstract

Stars with the B[e] Phenomenon. ASP Conference Series, Vol. 355, Proceedings of the Conference Held 10-16 July, 2005, at the Isl

Astronomy and Astrophysics

Astronomy

Scientific paper

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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