Star Formation in Young Universe
Super star clusters (SSCs) are thought to be the progenitors of globular clusters and represent the densest star-forming environments in the Universe. Strong gravitational lensing offers us a natural microscope to study individual newborn SSCs during Cosmic Noon (z=2-3) when the Universe was a factor of few smaller than it is today.
In a latest work led by Berkeley gradudate student Massimo Pascale, our group analyzed and interpreted the stellar and nebular emissions from a ~3 Myr-old, very massive ( tens of millions solar masses) newborn SSC with escaping Lyman continuum radiation, in the Sunburst Arc (see Rivera-Thorsen et al). We found evidence for dense, radiatively-pressurized photoionized clouds surrounding the monster system at only several parsecs. We are surprised to find that these clouds have unusual chemical compositions such as a high level of nitrogen enrichment, which most likely originates from massive star ejecta.
Our findings have tantalizing implications for the long-standing puzzle of why globular clusters appear to consist of multiple stellar populations with distinct element abundances. We might be witnessing, in the first few million years of a compact massive starburst system, the making of self-enriched material which will later give birth to stars of unusual element abundances.