B[e] Supergiants in the Magellanic Clouds

Details B[e] Supergiants in the Magellanic Clouds B[e] Supergiants in the Magellanic Clouds

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..355..135z&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

11

Scientific paper

The B[e] supergiants in the Magellanic Clouds form a subgroup of 15 massive stars showing the B[e] phenomenon. The properties of the B[e] supergiants can be explained in terms of a two-component stellar wind model. From their position on the H-R diagram it is clear that B[e] supergiants are in a post-main sequence evolutionary stage. Recent observational results on several B[e] supergiants with relevance to the question of an evolutionary connection with the luminous blue variables are discussed.

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