“Supermassive Black Holes Ejected from Galactic Centers: Quasar Survey Supports 10-Year-Old” — what this page in the network covers. A new analysis of around 100,000 quasars by researchers at Eötvös Loránd University (ELTE) has uncovered statistical evidence that some supermassive black holes are ejected from the centers of their host galaxies. The study, which supports a prediction made a decade ago by ELTE scientists Peter Raffai and Zsolt Frei along with Zoltán Haiman, suggests that these colossal objects can be displaced after formation. Quasars—extremely luminous galactic cores powered by accreting supermassive black holes—serve as key tracers in this investigation.
The finding matters because it provides a potential explanation for the observed offset between quasar positions and their host galaxies, a phenomenon that has puzzled astronomers. By confirming the theoretical framework proposed in 2013, the research opens new avenues for understanding the dynamics of galaxy evolution and the role of gravitational recoil in shaping the universe. The full version stays on the original page, which this listing opens directly.
