  We present an analysis of the X-ray emission for a complete sample of 288
Abell clusters spanning the redshift range 0.016<= z <= 0.09 from the ROSAT
All-Sky Survey. This sample is based on our 20cm VLA survey of nearby Abell
clusters. We find an X-ray detection rate of 83%. We report cluster X-ray
fluxes and luminosities and two different flux ratios indicative of the
concentration and extent of the emission. We examine correlations between the
X-ray luminosity, Abell Richness, and Bautz-Morgan and Rood-Sastry cluster
morphologies. We find a strong correlation between Lx and cluster richness
coupled to a dependence on the optical morphological type. These results are
consistent with the observed scatter between X-ray luminosity and temperature
and a large fraction of cooling flows. For each cluster field we also report
the positions, peak X-ray fluxes, and flux-ratios of all X-ray peaks above
3-sigma significance within a box of 2x2 Mpc centered on Abell's position.
