We present a study of the distribution of AGNs in clusters of galaxies with a uniformly selected, spectroscopically complete sample of 35 AGNs in eight clusters of galaxies at z=0.06-->0.31. We find that the 12 AGNs with LX>10^42^ergs/s in cluster members more luminous than a rest-frame M_R_<-20mag are more centrally concentrated than typical cluster galaxies of this luminosity, although these AGNs have comparable velocity and substructure distributions to other cluster members.