Concurrent formation of supermassive stars and globular clusters: implications for early self-enrichment
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DOI: 10.1093/mnras/sty1059
Abstract: We present a model for the concurrent formation of globular clusters (GCs) and supermassive stars (SMSs, ≳103 M⊙) to address the origin of the HeCNONaMgAl abundance anomalies in GCs. GCs form in converging gas flows and… read more here.
Keywords: supermassive stars; concurrent formation; gas; formation ... See more keywords