CORDIS Project
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This research focuses on the dynamics of globular star clusters, particularly the presence of multiple stellar populations and their evolution. It aims to develop a new dynamical model by analyzing observational data and numerical simulations to understand the role of angular momentum and intermediate mass black holes.
In the last few years our traditional interpretative paradigm of the internal dynamics of globular star clusters (GCs) has been revolutionized by a series of discoveries about their chemical, structural, and kinematic properties.
The existence of multiple stellar populations is now regarded as a ubiquitous phenomenon, while for decades GCs have been viewed as the epitome of a “simple stellar population”.
Empirical scaling relations between super massive black holes masses and the veloc…
THE UNIVERSITY OF EDINBURGH
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