We present the first X-ray observations of the dwarf nova Z Cam taken
during outburst. ROSAT Survey observations show that Z Cam conforms to
the pattern of X-ray behaviour seen in other dwarf novae, i.e., the q
uiescent hard X-ray emission is suppressed during outburst and replace
d by extreme-ultraviolet emission which declines more rapidly than the
optical flux. The timing of the hard X-ray suppression is measured wi
th precision for the first time in any system.