“…The first indication that flare activity could be possibly used as a reliable criterion for determining the membership of stars in stellar systems was obtained from the discussion of the distribution of FSs in the Pleiades cluster region. Namely, the space distribution of FSs in the Pleiades cluster showed (e.g., Chavushian, 1979, Chavushian et al, 1999, 2004, Hambaryan, 1998, Mirzoyan, 1976, 1983 that the concentration of FSs around the center of the Pleiades cluster is the same, i.e. the surface density of FSs decreases upon distance from the center of cluster, irrespective their proper motion or membership probability.…”