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While several studies have investigated large-scale cluster winds resultingfrom an intra-cluster interaction of multiple stellar winds, as yet they havenot provided details of the bordering flows inside a given cluster. The presentwork explores the principal structure of the combined flow resulting from theinteraction of multiple stellar winds inside stellar clusters. The theory ofcomplex potentials is applied to analytically investigate stagnation points,boundaries between individual outflows, and the hydrodynamic structure of theasymptotic large-scale cluster wind. In a second part, these planarconsiderations are extended to fully three-dimensional, asymmetricconfigurations of wind-driving stars.  We find (i) that one can distinguish regions in the large-scale cluster windthat are determined by the individual stellar winds, (ii) that there arecomparatively narrow outflow channels, and (iii) that the large-scale clusterwind asymptotically approaches spherical symmetry at large distances. Thecombined flow inside a stellar cluster resulting from the interaction ofmultiple stellar winds is highly structured.

The interaction of multiple stellar winds in stellar clusters: potential flow