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Superbubble dynamics in globular cluster infancy II. Consequences for secondary star formation in the context of self-enrichment via fast rotating massive stars
Martin Krause, Corinne Charbonnel, Thibaut Decressin +2
The self-enrichment scenario for globular clusters (GC) requires large amounts of residual gas after the initial formation of the first stellar generation. Recently, Krause et al.…
How did globular clusters lose their gas?
C. Charbonnel, M. Krause, T. Decressin +3
We summarize the results presented in Krause et al. (2012) on the impact of supernova-driven shells and dark-remnant accretion on gas expulsion in globular cluster infancy.
Superbubble dynamics in globular cluster infancy I. How do globular clusters first lose their cold gas?
Martin Krause, Corinne Charbonnel, Thibaut Decressin +3
The picture of the early evolution of globular clusters has been significantly revised in recent years. Current scenarios require at least two generations of stars of which the fir…