Here we present a self-consistent stationary solution for sphericallysymmetric winds driven by massive star clusters under the impact of radiativecooling. We demonstrate that cooling may modify drastically the distribution oftemperature if the rate of injected energy approaches a critical value. We alsoprove that the stationary wind solution does not exist whenever the energyradiated away at the star cluster center exceeds ~ 30% of the energy depositionrate. Finally we thoroughly discuss the expected appearance of super-starcluster winds in the X-ray and visible line regimes. The three solutions herefound: the quasi-adiabatic, the strongly radiative wind and the inhibitedstationary solution, are then compared to the winds from Arches cluster, NGC4303 central cluster and to the supernebula in NGC 5253.
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