Finding evidence for self-enrichment and supermassive stars in forming globular clusters Self-enrichment is one of the leading explanations for chemical anomalies in globular clusters. In this scenario, a polluter star enriches a forming cluster with its yields, likely ejecting radioactive 26Al into its surroundings. Young massive star clusters, as potential...

Probing the Finely-Resolved 100 TeV Gamma-Ray Sky for Ultra-Heavy Dark Matter - Dark100 abstract TBA