  A long BeppoSAX observation of the Galactic Center region shows that the
spectrum of the diffuse X-ray emission from the SgrA Complex can be described
with the sum of two thermal plasma models with temperatures of ~0.6 keV and
\~8-9 keV. The spatial distribution of the diffuse emission is energy
dependent. While the hard X-ray emission has a nearly symmetric distribution
elongated along the Galactic Plane, the soft X-rays (E < 5 keV) are remarkably
well correlated with the triangular radio halo of SgrA East. The parameters
derived for the soft component support the interpretation of the SgrA East
shell in terms of an evolved supernova remnant.
