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The B[e] stars

Published online by Cambridge University Press:  12 April 2016

F.-J. Zickgraf
F.-J. Zickgraf*
Affiliation:
Landessternwarte Königstuhl D-6900 Heidelberg 1

Abstract

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B[e] supergiants show evidence for a non-spherical two-component stellar wind. The general appearance and the physical properties of the suggested disk-like configuration are discussed. The high mass-loss rates, the surprisingly large number and the location in the H-R diagram make these stars important for the understanding of the post-main-sequence evolution of massive stars.

Type
Section I: Main Papers, General Discussions, and Two Panel Discussions
Information
International Astronomical Union Colloquium , Volume 113: Physics of Luminous Blue Variables , 1989 , pp. 117 - 120
Copyright
Copyright © Kluwer 1989

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