Computer simulations show how mysterious intermediate-mass black holes could form inside stellar clusters.
An international consortium of astronomers, including staff from the Max Planck Institute for Astronomy, has successfully unraveled the intricate formation mechanisms of the elusive intermediate-mass black holes. They could represent the link between their smaller relatives, the stellar black holes, and the supermassive giants that populate the centers of galaxies. This achievement derives from the DRAGON-II simulation project led by the Gran Sasso Science Institute. The scientists involved in this study computed the complex interactions of stars, stellar black holes, and physical processes inside dense stellar clusters, demonstrating that black holes of up to a few hundred solar masses can emerge in those environments.
The Cradle of Black Holes.
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