  We report on the analysis of the ASCA and BeppoSAX X-ray observations of the
polar system BL Hyi. Emission from both poles is apparent in both observations;
the emission from the second pole varies from cycle to cycle, indicating
non-stationary accretion there. The temperature of the post-shock region is
estimated to be about 10 keV. Inclusion of both complex absorption and Compton
reflection significantly improves the quality of the fit. No soft X-ray
component is observed; the BeppoSAX/LECS upper limit to the soft component is
in agreement with theoretical expectations for this low magnetic field system.
