THE CORRELATION-FUNCTION OF FLUX-LIMITED X-RAY-CLUSTERS

We show that the spatial correlation function of a flux-limited sample of X-ray selected clusters of galaxies will exhibit a correlation sca le that is smaller than the correlation scale of a volume-limited, ric hness-limited sample of comparable apparent spatial density. The flux- limited sample contains clusters of different richnesses at different distances: poor groups are found nearby and rich clusters at greater d istances. Since the cluster correlation strength is known to increase with richness, the flux-limited sample averages over the correlations of poor and rich clusters. On the other hand, a volume-limited, richne ss-limited sample has a minimum richness threshold, and a constant mix ture of richnesses with redshift. Using the observed correlation scale for rich (R greater-than-or-equal-to 1) clusters, r0(R greater-than-o r-equal-to 1) = 21 +/- 2 h-1 Mpc, that was determined from previous vo lume-limited studies, we derive for the ROSAT flux-limited X-ray clust er sample r0 (flux-limited) almost-equal-to 14 h-1 Mpc, in agreement w ith the recently observed value of 13.7 +/- 2.3 h-1 Mpc.