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Rotation of B[e] Supergiants, Luminous Blue Variables and Wolf-Rayet Stars

Published online by Cambridge University Press:  26 May 2016

Philippe Eenens
Philippe Eenens*
Affiliation:
Departmento de Astronomía, Universidad de Guanajuato, Apartado 144, Guanajuato, Gto 36000, Mexico & Institut d'Astrophysique, Université de Liège, Belgium

Abstract

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A brief review of the observational properties of evolved massive stars is presented. In the pursuit of clues for their rotation, formidable difficulties are encountered. At the same time, common features emerge between B[e] supergiants, Luminous Blue Variables and Wolf-Rayet stars. Several indications of rapid rotation are found, mostly indirect ones, in each class. It is shown that fast rotation can probably survive the mass loss events which characterize the late evolution of massive stars.

Information

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 97 - 106
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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