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S Doradus Type; Hubble-Sandage Variables

Published online by Cambridge University Press:  04 August 2017

B. Wolf
B. Wolf*
Affiliation:
Landessternwarte, Königstuhl, 6900 Heidelberg, West Germany

Abstract

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The luminous S Dor variables or Hubble-Sandage variables have gained considerable interest during the past few years for their exceptional (if compared to normal luminous hot stars) stellar wind properties. They seem to represent a short intermezzo in the evolution of the very massive stars prior to becoming WR stars. More recent results on S Dor variables (mainly of the LMC) are briefly summarized. Since most of the data have been or are going to be published elsewhere only an outline will be presented here.

Type
Session 3. Luminous Blue Variables
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 151 - 156
Copyright
Copyright © Reidel 1986 

References

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