  CH Cygni is a symbiotic star consisting of an M giant and an accreting white
dwarf, which is known to be a highly variable X-ray source with a complex,
two-component, spectra. Here we report on two Suzaku observations of CH Cyg,
taken in 2006 January and May, during which the system was seen to be in a soft
X-ray bright, hard X-ray faint state. Based on the extraordinary strength of
the 6.4 keV fluorescent Fe K-alpha line, we show that the hard X-rays observed
with Suzaku are dominated by scattering.
