From time to time, the black hole at the center of an HCSS will disrupt a star that passes too close, producing a very luminous flare. A few such flares have been observed at the centers of galaxies, presumably caused by a star coming too close to the SMBH in the galaxy nucleus. It has been estimated that a recoiling SMBH will disrupt about a dozen stars during the time it takes to escape from its galaxy. Since the lifetime of a flare is a few months, the chances of seeing such an event are small unless a large volume of space is surveyed. A star in a HCSS could also explode as a Type I (white dwarf) supernova.