The Pressure-confined Wind of the Massive and Compact Super Star Cluster M82-A1
The observed parameters of the young super star cluster M82-A1 and its associated compact H II region are here shown to indicate a low heating efficiency or immediate loss, through radiative cooling, of a large fraction of the energy injected by stellar winds and supernovae during the early evolution of the cluster. This implies a bimodal
Silich, Sergiy et al.
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11
2007