G. Maravelias, M. Kraus, A. Aret
Published 2015-07-30Version 1
B[e] supergiants are evolved massive stars with a complex circumstellar environment. A number of important emission features probe the structure and the kinematics of the circumstellar material. In our survey of Magellanic Cloud B[e] supergiants we focus on the [OI] and [CaII] emission lines, which we identified in four more objects.
Comments: 2 pages; 1 figure; submitted to the proceedings of the Physics of Evolved Stars - A conference dedicated to the memory of Olivier Chesneau, Nice, France, June 8-12, 2015
B[e] Supergiants' circumstellar environment: disks or rings?
New mass-loss rates of Magellanic Cloud B supergiants from global wind models
Resolving the kinematics of the disks around Galactic B[e] supergiants
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