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X-ray Emission from Isolated Be Stars

David H. Cohen
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Abstract

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.

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David H. Cohen. 2000-08-22. X-ray Emission from Isolated Be Stars. https://arxiv.org/abs/astro-ph/0008346

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