  As part of the Chandra GTO program we are monitoring and surveying M31 using
the HRC and ACIS cameras. These observations have resolved the nuclear X-ray
source into five separate sources, one of which is very soft and may (or may
not!) be associated with the central super-massive black hole. In addition, the
superb spatial resolution and low scattering of the Chandra telescope allows us
to unambiguously resolve the diffuse emission from the point sources. This
emission is clearly softer than the point sources, and also increases with
temperature radially. The monitoring nature of the observations allows detailed
study of the variability of the point sources.
