CTIO  > Science Talks  >  Abstracts

 

Santi Cassisi
Osservatorio Astronomico di Teramo, Italy
& NOAO South Visiting Astronomer
 


"Multiple Stellar Populations in Galactic Globular Clusters: Empirical Evidence and Theoretical Insights"
 

It had always been considered that the value of studying GCs is that they host simple, single stellar populations, i.e., that stars belonging to the same cluster share the same distance, age and chemical composition. However, in recent times, on the basis of accurate photometric and spectroscopic investigations, several exciting results have been obtained, such as the existence of anti-correlations between some chemical elements, the presence of multiple stellar populations in the same cluster, and peculiar features along the Horizontal Branch. Many of these outcomes severely challenge our understanding of stellar evolution and of evolution/formation mechanism of stellar clusters.
We review the main anomalies, recently observed in galactic GCs, and discuss the main evolutionary scenari suggested for interpreting these empirical evidence.