A missing link in black hole evolution

Research report (imported) 2024 - Max Planck Institute for Astronomy

Authors
Häberle, Maximilian; Neumayer, Nadine; Pössel, Markus; Nielbock, Markus
Departments
Max-Planck-Institut für Astronomie, Heidelberg
Summary
We have identified rapidly moving stars in the Omega Centauri star cluster, indicating the presence of a black hole at its centre with a mass of at least 8,200 solar masses. While astronomers had long assumed such intermediate-mass black holes exist, there has been a lack of reliable observations to confirm it. This discovery also establishes that Omega Centauri is the core region of a galaxy absorbed by the Milky Way billions of years ago. Stripped of its outer stars, the galactic core has since undergone little further evolution.

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