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Winds and outflows are ubiquitous at several scales throughout the Cosmos.
They often develop a bubble structure characterized by strong shocks and turbulence where high-energy particles can be efficiently produced.
I will present a model in which diffusive shock acceleration is a key process to energize particles in such astrophysical winds.
I will show some model applications in the context of young massive stellar clusters, starburst galaxies and active galactic nuclei and
I will discuss the associated multi-messenger implications in terms of high-energy photons, neutrinos and escaping cosmic rays.