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Center for Nonlinear Studies |
Globular Clusters (GCs) are often thought of as simple stellar populations, whose stars all have identical compositions and ages, but recent data have made it clear that this picture is inaccurate. I will present a new model in whichwell-known clumpiness in star-forming regions leads to more complex abundance patterns, as observed, and discuss how to use this new model to better understand the original properties of proto-GC molecular clouds and the fossilhistory of the Milky Way.
Host: Jonas Lippuner