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X-ray Emission from Isolated Be Stars

Published online by Cambridge University Press:  12 April 2016

David H. Cohen
David H. Cohen*
Affiliation:
Bartol Research Institute, University of Delaware, Newark, DE 19716

Abstract

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I discuss the X-ray observations of Be stars, and how their properties compare to non-emission B stars. I focus on several specific stars that show high flux levels and variability but also report on several interesting survey results. The Be X-ray properties are discussed in the context of wind-shock X-ray emission from normal OB stars as well as in the context of general mechanisms that have been proposed to explain the Be phenomenon. Finally, I conclude with a discussion of the spectral diagnostics that will be available from the new generation of X-ray telescopes.

Type
2. New Missions
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 156 - 169
Copyright
Copyright © Astronomical Society of the Pacific 2000

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