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start [2017/05/05 13:55]
start [2018/04/18 18:54]
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 +<slider :​sms_schematic.png>​
 +**A new self-enrichment model for globular clusters**
 +New model for the origin of multiple stellar populations in globular clusters: a supermassive star forms at the same time as the cluster and "​pollutes"​ the low-mass stars that survive until today in the first few Myrs. Key points: only a single generation of stars is needed, there is no mass budget problem and we provide testable predictions for observer: ​ [[https://​arxiv.org/​abs/​1804.04682v1]]. ​
 <slider :​eriii.png>​ <slider :​eriii.png>​