  We report on the Chandra ACIS-S3 imaging observation of the globular cluster
NGC 6752. We detect 6 X-ray sources within the 10.5" core radius and 13 more
within the 115" half-mass radius down to a limiting luminosity of Lx approx
10^{30} erg/s for cluster sources. We reanalyze archival data from the Hubble
Space Telescope and the Australia Telescope Compact Array and make 12 optical
identifications and one radio identification. Based on X-ray and optical
properties of the identifications, we find 10 likely cataclysmic variables
(CVs), 1-3 likely RS CVn or BY Dra systems, and 1 or 2 possible background
objects. Of the 7 sources for which no optical identifications were made, we
expect that ~2-4 are background objects and that the rest are either CVs or
some or all of the five millisecond pulsars whose radio positions are not yet
accurately known. These and other Chandra results on globular clusters indicate
that the dozens of CVs per cluster expected by theoretical arguments are being
found. The findings to date also suggest that the ratio of CVs to other types
of X-ray sources is remarkably similar in clusters of very different structural
parameters.
