  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.
