How did globular clusters lose their gas?
C.Charbonnel, M.Krause, T.Decressin, G.Meynet, N.Prantzos, R.Diehl

TL;DR
This paper reviews mechanisms like supernova-driven shells and dark remnant accretion that influence how globular clusters lose their gas during early development stages.
Contribution
It synthesizes previous findings on gas expulsion processes in globular clusters, highlighting the roles of supernovae and dark remnants.
Findings
Supernova-driven shells contribute significantly to gas expulsion.
Dark remnant accretion impacts gas retention in clusters.
Multiple mechanisms work together to clear gas from globular clusters.
Abstract
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.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies
