A black hole once believed to bridge the gap between stellar-mass and supermassive black holes has been re-evaluated. The object, previously identified as an intermediate-mass black hole in the dense star cluster Omega Centauri, has been reclassified as a cluster of smaller stellar-mass black holes. This finding challenges earlier conclusions about the discovery of this elusive category of black holes. Omega Centauri, located within the Milky Way and containing around 10 million stars, has long been studied for its unique characteristics and potential remnants of a cannibalised dwarf galaxy. Analysis of Omega Centauri According to researchers, as reported by Live Science, the identification was based on unusual stellar velocities within Omega Centauri’s core. These movements were initially attributed to an intermediate-mass black hole, estimated at 8,200 solar masses, observed using the Hubble Space Telescope. The new study, however, factored in pulsar data, leading to the revised conclusion. Pulsars, rapidly rotating neutron stars emitting radiation beams, provided detailed insights into the cluster’s gravitational forces. Justin Read, a researcher at the University of Surrey, has stated to …