  Intermediate and massive stars drive fast and powerful isotropic winds that
interact with the winds of nearby stars in star clusters and the surrounding
interstellar medium (ISM). Wind-ISM collisions generate astrospheres around
these stars that contain hot $T\sim 10^7$ K gas that adiabatically expands. As
individual bubbles expand and collide they become unstable, potentially driving
turbulence in star clusters. In this paper we use hydrodynamic simulations to
model a densely populated young star cluster within a homogeneous cloud to
study stellar wind collisions with the surrounding ISM. We model a
mass-segregated cluster of 20 B-type young main sequence stars with masses
ranging from 3--17 $M_{\odot}$. We evolve the winds for $\sim$11 kyrs and show
that wind-ISM collisions and over-lapping wind-blown bubbles around B-stars
mixes the hot gas and ISM material generating Kolmogorov-like turbulence on
small scales early in its evolution. We discuss how turbulence driven by
stellar winds may impact the subsequent generation of star formation in the
cluster
